WD0000-014 See also (RF)(RS) WD0000-345 See also (OJ) WD0001+433 See also (QM)(RK) WD0002+165 See also (PP) WD0003-570 WD0003-570 consists of a non-magnetic WD and a late-type cool dwarf. (GU) WD0004+330 See also (QP)(QM)(NB)(NL)(RK) WD0005+511 Similar to the PG1159 degenerates but fewer, weaker metals and Balmer emission,X-ray corona,mass loss, Ref.(60)(84)(SM). WD0005-163 Temperatures ambigious. Ref.(PP) WD0005-267 PCEB. Ref.(QH). WD0008+424 See also (PV)(OJ) WD0009+501 WD0009+501 is a magnetic degenerate,the first known below 100 kilogauss, Ref.(9W)(9V) See also (PV)(OL)(OJ)(MV)(NB)(RQ) WD0010-000 See also (NC) WD0011-134 LHS1044 is a magnetic degenerate, Ref.(31) See also (PV)(MV)(NN)(OJ) WD0012+008 See also (OY) WD0013+008.1 See also (NC) WD0014+003 See also (QJ)(NC) WD0014-006 See also (QJ)(NC) WD0014-015 See also (MS)(NR) WD0015+004 See also (MV) WD0015-004 See also (PJ)(NC) WD0016+000 See also (QJ) WD0016-220 See also (PP) WD0016-258 Long period ZZ Ceti (OC) WD0018+147 See also (PD)(MV) WD0018-267 See also (OL) WD0019-105 Double-degenerate merger system. Ref.(QT). WD0019-113 See also (QJ) WD0019-287 ZZ Ceti candidate (HC) WD0022+274 See Also (PR) WD0022-400 CPMB with APMPN 0025-3949A as second component (IN). WD0023+144 See also (NC) WD0023+388 Triple star system, also identifies G171-B10B as the WD and G171-B10A as the MS. Ref.(MK) Likely closer to d~60pc Ref.(MQ) See also (QR)(QP) WD0023-109 Mis-identified as WD0023+109 in REf.(NZ) CPMB system with the K-star G158-077. Ref.(OF) Likely triple system - DA+dM0(G158-78B)+DC8(G158-78C). Ref.(PS) WD0024-010 See also (NC) WD0024-556 See also (PP) WD0025+000 See also (QJ)(NC) WD0025-004 See also (QJ)(NC) WD0025-277 ZZ Ceti candidate (HC) WD0027+151 See also (RS) WD0027-549 See Also (PR) WD0027-636 See also (QM)(PP)(JV)(RK) WD0028-274 See section A1.2 in Ref. (LJ). WD0028-474 Double-lined double-degenerate binary. Ref.(PP) WD0029+571 PG1159-like central star of SH2-136.(66). WD0029-181 See also (PP) WD0030+006 See also (NC) WD0030+444 Binary (DA5+G8) system. Ref.(MK) WD0030-001 See also (NC) WD0031-311 See also (PP) WD0032-175 See also (MR)(OH) WD0033+016 See also (PP)(MY) WD0033-007 See also (NC) WD0034+002 See also (PY) WD0034+008 See also (NC) WD0034-211 Close double degenerate binary, Ref.(45),(MQ) MS companion= LTT 0329B See also (MY) WD0036+312 Short period ZZ Ceti (OC) WD0037+312 See also (JV)(NL) WD0037-006 Double-lined double-degenerate binary. Ref.(PP) See also (OK) WD0038+555 G218-008 has strong UV absorption features, Ref.(CG). WD0038-226 LHS 1126 is the only know white dwarf to show JHK absorption, strong C2? H2? opacity, Ref.(DQ)(5X) See also (PV)(OL)(OJ)(MM) WD0039+149 See also (NC) WD0040+000 See also (PD) WD0041+092 Hot DA companion to the rapidly rotating K1-3V star BD+08 102, REF.(82)(4D). WD0041-102 FEIGE 7 is a magnetic white dwarf, Ref.(5F)(03). WD0044-121 NGC246 is a PG1159 star with several detected periods and an associated planetary nebula; type lgE, Ref.(66) Non-radial g-mode pulsator Ref.(KO)N. WD0045+000 See also (NC) WD0046+051 VAN MAANEN2 was the only example of a DG white dwarf, Ref.(DB) See also (PV)(2L)(NN)(OE)(OJ) WD0047+190 See also (QV)(MR) WD0047-524 See also (PP)(NL) WD0048-202 Possible sdOB/WD binary system. Ref.(QX). WD0048-294 See also (JV) WD0048-544 See also (PP) WD0049-011 See also (NC) WD0050-011 Post-common envelope binary. Ref.(QB)See also (QJ)(NC)(QH) WD0050-332 See also (PP)(JV)(MV)(NB)(NL)(RK) WD0051+006 See also (QJ) WD0052+004 See also (NC) WD0052-006 See also (QJ)(PE)(NC) WD0052-101 See also (OK) WD0053-103 See also (NC) WD0054-004 Reclassified as M star; Ref.(QB) WD0055+006 MS+MS superposition; Ref.(QB) WD0057+003 See also (NC) WD0058+148 See also (QJ)(NC) WD0058-044 See also (PP) WD0059-008 ZZ Ceti star Ref.(KB) WD0101+002 See also (QJ)(NC) WD0101+003 See also (QJ)(NC) WD0101+048 Double degenerate system. Ref.(JP)See also (PP)(OJ)(MM)(NB)(NL)(OL) WD0101+059 See also (MY) WD0101+866 See Also (PR) WD0101-182 See also (QC) WD0103-013 See also (RF)(RS) WD0104-102 Shortest period (39.1 min) detached WD binary system known. Ref.(SU) WD0104-464 BPM30551 is a ZZ CETI variable, Ref.(2W)(7I). See also (PB) WD0106-328 See also (PS)(PP) WD0106-358 Possible companion Finding chart for GD 683B see A4.2 in Ref.(LJ) See also (PP)(RK) WD0107+131 WD/MS eclipsing binary system. Ref.(PH) See also (NC)(QH)(QN) WD0108+000 ZZ Ceti star Ref.(KB) WD0108+143 See also (PP)(OK) WD0108+277 Cool Da with no metal features C. Melis 2008 private communication See also (PV)(PS)(OJ) WD0108-001 See also (QJ)(NC) WD0108-014 See also (QJ) WD0108-106 See also (NC) WD0110-139 See also (PP) WD0110-162 See also (PP) WD0111+002 See also (QP) WD0111-102 See also (RF)(RS) WD0112+132 See also (NC) WD0113+006 See also (NC) WD0114+002 See also (NC) WD0115+159 G033-049 has strong UV absorption features, Ref.(BO)(NB) See also (PO)(OJ). WD0116-231 Name(s) for MS companion(s). GD 695B See also (QP) WD0120+154 See also (NC) WD0120-024 See Also (PR) WD0121-006 See also (QJ) WD0121-429 Magnetic DA+DC double degenerate. Ref.(MD)(NY) See also (OJ) WD0121-756 See also (JV)(KL)(SM) WD0122+200 Pulsating PG1159 DO degenerate, Ref.(DN)(39); TYPE A, Ref.(66) Non-radial g-mode pulsator Ref.(KO)N. WD0124-257 See also (PP) WD0126+101 Double degenerate system. Ref.(JP) See also (PP)(MM)(NB)(OL)(RQ) WD0127+581 The DAO central star of the planetary nebula Sh2-188, Ref.(7U) WD0127-311 HE0127-311 is a magnetic degenerate, Ref.(3W). WD0128-012 See also (NC) WD0128-387 MCT0128-3846 is an unresolved DA + DB or DBA binary. (DM) WD0129-205 See also (PP) WD0130+128 See also (QJ)(NC) WD0130+141 See also (NC) WD0130-196 MCT0130-1937 is a PG1159 star with no detected variability, type A, Ref.(66). WD0130-273 See also (PP) WD0131-163 See Section A5.16 in Ref.(LJ) See also (QP)(PP)(JV)(MQ)(MY)(NL)(RK) WD0131-287 ZZ Ceti candidate (HC) WD0132+127 Spectrum shows Mg I, Ref.(JJ) WD0133-116 R548 is a ZZ CETI variable, Ref.(5C) See also (PP)(NL) WD0133-299 ZZ Ceti candidate (HC) WD0134+181 See also (JE) WD0134+833 See also (QP)(NB)(NL) WD0134-002 See also (QJ)(NC) WD0135+002 See also (QJ) WD0135-052 LP870-2 is a close detached DA binary system, Ref.(9K) Radial velocities -16.6/-41.2 km/sec Ref.(JP)N See also (NL)(OE)(OJ) WD0136+251 Hot, low field magnetic ultra-massive DA star, Ref.(5V) See also (OQ)(9U)(JV)(NL)(RK) WD0136+768 Double-degenerate system. Ref.(QX). WD0136-201 Single-lined double-degenerate binary. Ref.(PP) WD0137-004 See also (NC) WD0137-349 Binary system consisting of a DA and a very low-mass detached companion. Ref.(RO).See also (QH)(SE) WD0139+143 See also (NC) WD0139+513 NGC650-1 is a PG1159 star with no detected variability and an associated planetary nebula, type E, Ref.(66). WD0139-011 See also (QJ)(NC) WD0140+130 See also (MV) WD0141-675 See also (OJ)(MV)(MM)(OL)(RQ) WD0143+216 See also (PP)(MY) WD0145-174 See also (NN) WD0145-221 ZZ Ceti star ref.(JT) Has a possible Brown Dwarf Companion ref.(KX) See also (QP)(PP) WD0145-257 Name(s) for MS companion(s). GD1401B See also (QP) WD0146+187 See also (QA)(PS) WD0147+674 See also (RK) WD0148+467 1400A absorption feature, Ref.(CL) Member of binary or multiple star system. Ref.(OJ) See also (PV)(PO)(NB)(NL) WD0148+641 GR268 common proper motion binary with G244-37 (M2 DWARF), Ref.(1R). WD0149-012 See also (NC) WD0149-082 See also (NC) WD0150+001 See also (NC) WD0150+007 See also (PY) WD0150-089 See also (PE) WD0151+017 See also (PP) WD0151-308 See also (QV) WD0154-071 See also (QC) WD0155+003 Spectrum shows Mg I, Ref.(JJ) WD0155+069 See also (PS) WD0156+155 See also (PS) WD0158+235 A new hot DO with ultra highly excited ionization stages, Ref.(64). WD0158-160 Composite DBA + dM binary, Ref.(DP). WD0159-032 WD0159-032 is a magnetic degenerate, Ref.(02). WD0201+004 See also (NC) WD0201-006 See also (NC) WD0201-052 See also (PP) WD0202-055 See also (PF) WD0203+007 Reclassified as carbon star; Ref.(QB)See also (NC) WD0203+131 See also (NC) WD0203-010 See also (NC) WD0203-138 See also (PP) WD0204-233 See also (PP) WD0204-306 CPM Binary with LP885-923 (WD+dM) Ref.(MK)(PR) WD0205+000 See also (NC) WD0205+133 Name(s) for MS companion(s). PG 0205+133B See also (QR)(QP) WD0205+250 See also (NL) WD0205-297 Double-lined double-degenerate binary. Ref.(PP) WD0208+002 See also (PD)(MV) WD0208+396 G74-7 is the first known example of a definite DA, F degenerate, REF.(37),See also (QV)(QA)(MR)(NN)(RT) WD0208-153 Name(s) for MS companion(s). MRT 0208-1520B WD0208-510 CMPB with the dK1 Gliese 86; the WD Gl 86B Should not be confused with the exolanet GJ86b. Ref.(SB).See also (RZ) WD0209+085 DAB star in the DO-DB gap, Ref.(63), Teff=36,000K, Ref.(3X),(63) See also (QP)(PP) WD0209+210 See also (PD)(MV) WD0210+000 See also (NC) WD0210+086 White dwarf companion to the mild barium star XI 1 CETI; DA4 with 1400 and 1690 features, Ref.(37). Coords corrected, formerly WD0207+083 WD0210+138 See also (NC) WD0210+168 See section A1.3 in Ref. (LJ). WD0210-010 See also (NC) WD0211+010 See also (QJ)(NC) WD0211-086 ZZ Ceti star Ref.(KB) See also (NQ) WD0212+140 See also (NC) WD0213+396 See also (MY) WD0213+427 See also (OJ)(NN) WD0214+568 See also (MZ)(NL) WD0214-007 See also (QJ)(NC) WD0215+005 See also (QJ)(NC) WD0215+006 See also (QJ)(NC) WD0216+007 See also (NC) WD0216+143 See also (QP)(PP)(JE) WD0216+387 See also (PQ) WD0216-005.1 See also (QJ)(NC) WD0216-032 Luminosity of white dwarf probably dominated by wind accretion energy, Ref.(BX)(JV)(SM). WD0217+003 See also (QJ) WD0218+000 See also (NC) WD0219+282 Has an Unresolved companion DA1.9 White Dwarf with (Vmag = 18.16 AbsMag = 10.32) Ref.(QC) Triple-star system: (DA+DB)+dM5 companion. Ref.(QO)(SG) WD0220+222 See also (PP)(PQ)(SM) WD0221+399 SEE also (PR) WD0221+399 CPM Binary with BD+39 0539 (WD+dM) system. Ref.(MK) WD0222+006 See also (QJ)(NC) WD0222+422.1 CPM WD component with Mv > 15.0, Ref.(3A). WD0222+422.2 CPM WD component with Mv > 15.0, Ref.(3A). WD0222+648 Mv > 15.0, Ref.(51) formely WD0222+641. WD0222-291 We obtain T=3000 K, this may be the coolest WD known. (JW). WD0225-192 Double-lined double-degenerate binary. Ref.(PP) WD0226-078 See also (QJ) WD0227+001 See also (QJ) WD0227+009 See also (NC) WD0227+050 See also (PP)(NB)(NL) WD0228-009 See also (NC) WD0228-085 DB; binary nature questionable.Ref.(QB)See also (NC) WD0229+270 See also (QC) WD0230+343 See also (RY) WD0230-144 See also (PV)(OJ) WD0231-054 See also (MY)(NL) WD0232+035 FEIGE 24 is an EUV source, PCEB, DAQZ+dwarf M2, Ref.(RV)(5Y) See also (QH)(PP)(NL)(RX)(SM). WD0232+525 See also (NL) WD0232-003 See also (QJ)(PJ)(NC) WD0233-083.1 See also (MV) WD0233-242 See also (OJ) WD0234-012 See also (NC) WD0235+064 CPMB system (DAZ+dM3.5 companion). Ref.(PS)See also (QA) WD0235-003 See also (QJ)(NC)(QH) WD0235-125 See also (RL)(RK) WD0236+498 See also (NO)(RK) WD0237+105 Single-lined double-degenerate binary. Ref.(PP) WD0237+115 Name(s) for MS companion(s). PG 0237+115B WD0239+109 G4-34 is a probable unresolved DA + DB binary, Ref.(23). WD0240+004 See also (QJ)(NC) WD0242+002 See also (QJ)(NC) WD0242+009 See also (QJ)(NC) WD0243-026 See also (QV)(QA)(OJ)(MR)(RT) WD0244+004 PCEB. Ref.(QH) See also (QJ)(NC) WD0245+541 See also (QA)(OJ)(MR)(RT) WD0246+326 ZZ Ceti star ref.(GX) WD0246-301 ZZ Ceti candidate (HC) WD0247+053 A new DBA star from the HS survey, Ref.(4B) WD0248-014 See also (NC) WD0249-002 See also (NC) WD0250-007 CPMB with BD-01 0407 Ref.(EP), Referenced as 0250-008 in Ref.(MK)(PR) WD0251-008 See also (PQ) WD0252-009 See also (NC) WD0252-055 EUVE-discovered hot DA companion to the K0 IV star HD18131, Ref.(4D),(BP). WD0252-350 See also (PP) WD0253+508 New magnetic degenerate, Ref.(61). WD0253-070 See also (NC) WD0253-077 See also (QJ)(NC) WD0255+006.1 See also (NC) WD0255+009.2 See also (NJ)(NC) WD0255-007 See also (PJ)(NC) WD0255-110.1 See also (PP) WD0255-705 See also (PP)(OJ)(MV)(NB)(NL) WD0256-014 See also (QJ) WD0257+080 See also (MV) WD0257-005 Name(s) for MS companion(s). KUV 02579-0036B See also (QP) WD0257-075 See also (RF)(RS) WD0259+004 See also (NC) WD0300+007 WD/MS eclipsing binary system. Ref.(PH) See also (PH)(NC) WD0300-008 See also (QJ) WD0300-013 A DB degenerate with calcium, Ref.(AC). See also (QD)(QA)(PZ)(OR)(RF)(RS) WD0300-066 See also (NC) WD0301+004 See also (QJ)(NC) WD0301-006 See also (PD)(MV) WD0302+027 See also (QP)(PP)(NL)(RK) WD0302+621 See also (MU) WD0303-007 Name(s) for MS companion(s). KUV 03036-0043B See also (QP) WD0303-080 See also (QJ)(NC) WD0304+004 See also (NC) WD0304+154 See also (JV) WD0306-006 See also (QJ)(NC) WD0306-012 See also (NC) WD0307+077 See also (QV)(MR) WD0307-428 WD0307-428 is a magnetic degenerate, Ref.(02). WD0308+096 The dM companion is likely a binary M2 dwarf, see A5.19 in Ref.(LJ) See also (QX)(QX)(QH) WD0308+188 See also (QP) WD0309-005 See also (NC) WD0309-275 Name(s) for MS companion(s). WD 0309-75B WD0310-073 See also (OK) WD0310-688 1400A absorption feature, Ref.(CH) See also (PP)(NB)(NL)(OE)(OK) WD0311-013 See also (QJ)(NC) WD0313-066 See also (OY) WD0315-011 CPMB WITH BD-01 0469 See also (OS) WD0315-013 Double-lined double-degenerate binary. Ref.(PP) WD0316+003 ZZ Ceti star Ref.(KB) WD0316-003 See also (NJ) WD0316-849 RE0317-853 is a magnetic degenerate, Ref.(3Z). WD0317-011 See also (NC) WD0318-068 See also (QJ)(NC) WD0319-004 See also (QJ)(NC) WD0320-000 See also (OK) WD0320-192 Single-lined double-degenerate binary. Ref.(PP) WD0320-539 See also (PP)(JV)(NL)(RK) WD0321-002 See also (QJ)(NC) WD0321-009 Reclassified as QSO; Ref.(QB) WD0322+452 The DAO central star of HDW3, Ref.(7U). WD0322-013 See also (NC) WD0322-019 Double degenerate system. Ref.(JP)(NN) See also (QA)(OJ) WD0323+009 See also (NC) WD0324+738 RA=033013.89 Dec=+740157.1(2005.09), resolved triple (WD+dM5+dM6) system. Ref.(MQ) See also (QP) WD0324-012 See also (NC) WD0324-012.1 See also (NC) WD0324-197 Double-lined double-degenerate binary. Ref.(PP) WD0325-005 See also (QJ)(NC) WD0325-405 Single-lined double-degenerate binary. Ref.(PP) WD0325-857 LB 9802 is the visual companion to the high-field ultramassive WD EUVEJ0317-85.5, separation ~ 200AU. Ref.(MV)See also (RL) WD0326+001 See also (NC) WD0326-273 Double degenerate system; radial velocities 105.9/157.1 km/sec Ref.(JP) See also (PV)(OJ)(PR) WD0328+008 See also (PP)(PM)(OK) WD0328-010 See also (NC) WD0329+005 KUV03292+0035 is a magnetic degenerate, Ref.(3V). This star is listed at Dec -00 35.1 in Ref.(CP). See also (PD) WD0330-000 See also (PD) WD0330-009 See also (OK) WD0330-009.1 ZZ Ceti star Ref.(KB) WD0330-013 See also (NC) WD0331-356 Name(s) for MS companion(s). HE 0331-3541B See also (SM) WD0333+004 See also (QJ)(NC) WD0333-350 See also (JV) WD0334-002 See also (NJ) WD0334-009 See also (QJ)(NC) WD0335-002 See also (QJ)(NC) WD0335-420 See also (RK) WD0337+096 Hot/cold Table 1 temperatures ambigious. Ref.(PP) WD0338+007 See also (MS) WD0339+002 Has an Unresolved companion DB3.7 White Dwarf with (Vmag = 17.82 AbsMag = 11.57) Ref.(QC) WD0339-035 Temperatures ambigious. Ref.(PP) WD0339-451 See also (JV)(SM) WD0340+009 See also (QJ)(NC) WD0340-068 See also (PD)(MV) WD0340-075 See also (MS)(NR) WD0341+021 Variability in radial velocity indicates a long period binary. (EE) Single-lined double-degenerate binary. Ref.(PP) WD0341+182 See also (PV)(OJ)(NN) WD0341-076 See also (NC) WD0341-459 BPM31594 is a ZZ CETI variable, Ref.(7H). See also (PB) WD0342+004 See also (PD)(MV) WD0342+176 Double-degenerate merger system. Ref.(QT). WD0342+374 Hot DA planetary nucleus, Ref.(7U). WD0343+247 An ultra cool White Dwarf referred to in the references as WD0346+246 WD0343-007 See also (PP) WD0344+014 See also (OJ) WD0344+073 Long period ZZ Ceti (OC) single-lined double-degenerate binary. Ref.(PP) WD0344-121 See also (PP) WD0345+006 See also (RY) WD0345+498 IW1 is a PG1159 star with no detected variability and an associated planetary nebula, Ref.(DI); type A Ref.(66). WD0346-011 See also (PP)(OQ)(MY)(MZ)(NL)(RK) WD0346-063 See also (QJ)(NC) WD0347+171 V471 TAU,HYADES DA and K0V Eclipsing and Spectroscopic binary, REF(7V). DA star has TEFF=32,500K, LOG G=8, Ref.(2N)(JV). See also (PH)(SM) WD0347-137 Name(s) for MS companion(s). GD 051B See also (QP) WD0348+339 See also (NL) WD0348-066 See also (NC) WD0349+247 Pleiad white dwarf with mass 0.98 MSUN; VGRAV= +84+/- 9 KM/S, Ref.(CR) See also (OS)(OQ)(MZ) WD0350-002 See also (NC) WD0352+049 See also (PP) WD0352+096 The finding charts point to different stars. See also (PP)(OS)(OQ)(MZ)(NL) WD0354+463 See section A5.25 in Ref. (LJ), (MQ) See also (QP) WD0355+255 SEE also (PR) WD0357+081 See also (PF)(OJ) WD0357-233 Name(s) for MS companion(s). Ton S 392B See also (QP) WD0358-051 DA with odd H-Alpha emission; Ref.(QB)See also (NC) WD0400-346 CMPB with the G1/2 V double star HIP 18824. Ref.(SH) WD0401+149 Temperatures ambigious. Ref.(PP) WD0401+250 See also (NL) WD0406+169 See also (OS)(OQ)(NL) WD0408-041 Contains circumstellar dust (NG) See also (QV)(QD)(QA)(PS)(PP)(OR)(MR) WD0410+117 See also (QP)(PP)(NL) WD0410-116 Double-lined double-degenerate binary. Ref.(PP) WD0413-077 The mass of 40ERI B is 0.43 MSUN, Ref.(8K). 1400A absorption feature, Ref.(2A) CPMB with K1 V star HD 26965. Ref.(OF) See also (OS)(NL)(OK)(OJ)(RX) WD0415+271 HL TAU76 is a ZZ CETI variable, Ref.(4X). See also (PB)(OQ) WD0415-594 Sirius-like system. Ref.(RZ) CMPB with HD 27442A; the WD HD 27442B should not be confused with the exoplanet HD 27442b. Ref.(SA). WD0416+334 Finding chart for GD 60B Ref.(LJ) WD0416+402 See also (NO) WD0416-550 See also (PP)(JV) WD0417+361 G038-029 is a ZZ CETI variable, Ref.(7L). See also (PB) WD0418+137 Companion to HR 1358, a F6V spectroscopic binary. Ref.(EX)(SM) WD0419-487 Eclipsing system, WD + Red dwarf. See also (PH)(OJ)(MV)(QH)(SM) WD0420-007 See also (NC) WD0421+162 See also (PP)(OS)(OQ) WD0421+338 A quadruple system. (EX) WD0421+740 See also (QM)(RK) WD0422+543 See also (QX) WD0425+168 See also (QP)(PP)(OS)(OQ)(JV)(NL) WD0426+588 The mass of this star is 0.48 or 0.68 MSUN, Ref.(AW)(JV)(NN) See also(OJ). WD0429+176 White dwarf-red dwarf Hyades spectroscopic binary, REF(5B). DA white dwarf with T=20,000K, LOG G=8, Ref.(AR)(JV). See also (QH)(PP)(SM) WD0430+136 Name(s) for MS companion(s). KUV 04304+1339B/C. Triple-star system: Unresolved DA+dM4e binary and a dM5.5e companion. Ref.(QO) WD0431+126 See also (PP)(OS)(OQ) WD0433+270 EG40 common proper motion binary with G39-27 / BD+26 0730 (K5 DWARF), Ref.(7Z) See also (PV)(OJ)(PR). WD0435+410 See also (OB) WD0435-088 See also (OJ)(NN) WD0437+138 See also (OS)(OQ) WD0438+108 See also (QC)(OS)(OQ)(RY) WD0439+466 DAO nucleus of the planetary nebula S216, Ref.(7U). WD0440-038 See also (OQ)(JV)(RK) WD0443-275.1 Very close common proper motion pair, Ref.(7Z)(PR). WD0444+049 New PG1159 star, type A, Ref.(66). WD0446-789 See also (JV)(NB) WD0449-259 See also (OR) WD0453+418 See also (NL) WD0453-295 A rare DAB hybrid composition degenerate, Ref.(DP), MCT0453-295 is an unresolved DA + DB binary, Ref.(DM). WD0455+553 GR318 is a ZZ CETI variable, Ref.(7J). See also (PB) WD0455-282 A new hot DA in a region of extremely low HI density, Ref.(15) See also (NB)(NL)(RK) WD0455-532 single-lined double-degenerate binary. Ref.(PP) WD0457-004 See also (OJ) WD0457-103 K0IV + DA binary, Ref.(14). WD0458-665 X-ray selected hot DA + dM(RX J0458.9-6628B) binary, Ref.(3P)(SM). WD0500-156 The DAO central star of ABELL 7, Ref.(7U). WD0501+527 See also (QP)(PM)(NL)(OK)(RX) WD0501-289 Evidence of episodic mass ejection, rich metallic EUV spectrum, Ref.(DK,DT). WD0503-174 LHS1734 is a magnetic degenerate, Ref.(27)(MV) See also (PF)(OJ). WD0504-241 DO white dwarf with ultra-high excitation absorption, Ref.(31). WD0507+045.1 One component of a visual pair of DA stars, Ref.(63), ZZ Ceti star ref.(IY) See also (PB) WD0507+045.2 One component of a visual pair of DA stars, Ref.(63). See also (QP)(PP) WD0509-007 See also (PP)(MV)(NL)(RK) WD0510-418 See also (PP)(RK) WD0512+326 System of 4 stars; primary and tertiary components are spectroscopic binaries. Ref.(SI) See also (RK)(SM) WD0513+260 V1063 TAU is a non-radial pulsator, Ref.(44). See also (PB) WD0517+307 GD 66 is a ZZ CETI variable, Ref.(57). See also (PB) WD0517+357 PCEB. Ref.(QH). WD0518+333 Name(s) for MS companion(s). G086-B1A/C. Triple-star system: DA and a binary (dM3+dM3) proper motion companion. Ref.(QO)(PQ) WD0518-105 See also (OQ)(JV)(RK) WD0531-022 See also (JV) WD0532+414 Double degenerate system; radial velocities -38/150 km/sec Ref.(JP) See also (OJ) WD0532-560 ZZ Ceti star ref.(JT) WD0533+555 DA central star of the planetary nebula HDW4, Ref.(7U). WD0543+579 See also (MR) WD0548+000 See also (PP)(JV)(NL)(RK) WD0548+326 See also (OS) WD0548+326.1 See also (OS) WD0548-001 G99-37 is magnetic and polarized, Zeeman H alpha, Ref.(5H)(03) See also (PV)(MV)(OJ). WD0548-241 See also (RK) WD0549+158 See also (PP)(PM)(MV)(MZ)(NB)(NL)(RK) WD0549+324 See also (OS) WD0549+324.1 See also (OS) WD0549+325.1 See also (OS) WD0549+325.2 See also (OS) WD0549+325.3 See also (OS) WD0549+325.4 See also (OS) WD0549+325.6 See also (OS) WD0549+325.7 See also (OS) WD0549+326.1 See also (OS) WD0549+326.2 See also (OS) WD0551+123 CMPB with the F8 star HIP 27878. Ref.(SH) WD0552-041 See also (PC)(OJ)(MM)(NB)(NN)(OL)(RQ)(1V) WD0553+053 G99-47 is a magnetic white dwarf, Ref.(03) See also (OL)(MV)(MM)(NB)(NN)(OJ)(RQ). WD0556+106 Rare DA nucleus of planetary nebula with Teff > 1E+5K, Ref.(5J). WD0558-756 Helium-rich DO nucleus of K1-27; TEFF>1E+5;similar to KPD0005, Ref.(8O)(JV). WD0603-483 See also (NO)(RK) WD0605+241 NGC2168:LA 2 = NGC2168:LAWDS 2 WD0605+242 See also (OS) WD0605+245 NGC2168:LA22 = NGC2168:LAWDS22 See also (OS) WD0606+240 NGC2168:LA15 = NGC2168:LAWDS15 See also (OS) WD0606+241 NGC2168:LA11 = NGC2168:LAWDS11 WD0606+243 NGC2168:LA27 = NGC2168:LAWDS27 WD0606+244.1 NGC2168:LA 5 = NGC2168:LAWDS 5 See also (OS) WD0606+244.2 NGC2168:LA 6 = NGC2168:LAWDS 6 See also (OS) WD0612+177 G104-27 detection of trace helium in a DA star, Ref.(3K) See also (PP)(NL) WD0615+556 Central star of the planetary nebula PW1, Ref.(7U). WD0615-591 CPMB WITH CD-59 1275 See also (PR) WD0616-649 RE0616-649 is a new magnetic degenerate, Ref.(4A). WD0621-376 See also (QP)(PP)(MV) WD0622-329 Unresolved DA/DB double degenerate Ref.(MD) WD0625+415 Finding chart for GD 74B see A5.13 in (LJ) WD0625-253 Central star of Abell 15, REF.(2B). WD0630-050 See also (PP)(RK) WD0631+107 See also (RK) WD0637+477 GD77 is a magnetic degenerate, Ref.(9X) See also (MV) WD0640+015 Cool DO star (TEFF = 55000K) with one of the strongest HeII 4686 absorption lines of any known star, Ref.(7C)(5Q). WD0642-166 SIRIUS B mass=1.02 MSUN, Ref.(BK) See also (OS)(OJ). WD0642-285 CPMB WITH CD-28 3358 See also (PR) (P.Bergeron Finding Chart) WD0644+025 See also (OJ) WD0644+375 See also (OJ)(NB)(NL) WD0646-253 See also (MV)(RK) WD0651-020 See also (JV)(NL)(RK) WD0652-563 See also (OQ)(RL) WD0657+320 See also (OJ) WD0659-063 Listed in ref (NN) as WD0659-064 See also (OJ) WD0704+618 Coolest PG1159 star, no detected variability, Ref.(2T); type A, Ref.(66). WD0708-670 See also (PV) WD0710+216 See also (PP) WD0710+741 See also (QH) WD0713+399 A new DO star with ultra-highly excited ionization features, Ref.(31) WD0713-468 LONGMORE 3 is a PG1159 star with no detected variability and an associated planetary nebula, Ref.(7R)(KL). WD0714+458 Possible companion 0714+458 Finding chart for GD 84B see A4.1 in Ref.(LJ) WD0715-703 See also (JV)(MV)(NB)(RK) WD0718-316 DAO+dM2 pre-cataclysmic binary. Ref.(IT) See also (QM)(QH)(MV)(RK) WD0721-276 See also (MV)(RK) WD0726+133 ABELL 21 is a PG1159-like star with no detected variability and an associated planetary nebula Type E, Ref.(DG)(KL). WD0726+392 See also (PR) WD0727+376 See also (NC) WD0727+482 G107-70 consists of a close pair of DC stars, it is also a widely seperated CPM pair with a red subdwarf(G107-069) Ref.(AX)(NN) See also (OJ). WD0727+600 A new intermediate temperature DO star with ultra-highly excited species, Ref.(2T). WD0728+642 P. Bergeron reports his spectra does not show Zeeman splitting, Private Communication 3/11/2010 See also (OJ) WD0729+397 See also (NC) WD0730+487 See also (OQ) WD0732+330 See also (NC) WD0732-427 (P.Bergeron Finding Chart) WD0733+389 See also (NC) WD0733+468 MS+MS superposition; Ref.(QB) WD0734-143 See also (JV) WD0736+053 PROCYON B has mass =0.63 MSUN, Ref.(AV)(JV) See also (OJ)(SM). WD0736+278 See also (NC) WD0736+391 See also (NC) WD0737-384 Member of the open cluster NGC 2451, Ref.(4O). (P.Bergeron Finding Chart) WD0738+222 See also (NC) WD0738+283 See also (RS) WD0738+382 See also (NC) WD0738+418.1 See also (NC) WD0738-172 First detection of calcium two 1840A absorption in a white dwarf, Ref.(4L)(NN) LHS 234 M6.0V CPM companion(PC) See also (QA)(PO)(OJ). WD0738-382 Member of the open cluster NGC 2451, Ref.(4O). WD0739+238 See also (NC) WD0739+412 See also (NC) WD0740+325 See also (NC) WD0740+348 See also (NC) WD0741+248 See also (PR) WD0741+356 See also (NC) WD0742+231 See also (OK) WD0742+238 See also (NC) WD0742+653 A new intermediate temperature DO star, Ref.(2T). WD0743+442 See also (MY) WD0743+474 See also (NC) WD0743-336 VB3 common proper motion with HD63077 (G0 DWARF), shown to be low luminosity DC9 degenerate, not an M dwarf, Ref.(4T). (P.Bergeron Finding Chart) See also (OJ) WD0744+382 See also (NC) WD0744+384 See also (NC) WD0744+431 See also (QJ)(NC) WD0745+210 See also (NC) WD0745+247 See also (QJ)(NC) WD0745+258 See also (NC) WD0745+304 See also (PD)(MV) WD0745+436 See also (NC) WD0746+384 See also (NC) WD0746+396 See also (NC) WD0746-375 Member of the open cluster NGC 2451, Ref.(4O). WD0747+073.1 LHS 239 and LHS 240 are double DC white dwarfs, Ref.(5M)(NN) See also (OJ). WD0747+073.2 LHS 239 and LHS 240 are double DC white dwarfs, Ref.(5M)(NN) See also (OJ). WD0747+247 CPMB with WD 0747+247.1 Ref.(QL). WD0747+247.1 CPMB with WD 0747+247 Ref.(QL). WD0748+230 See also (NC) WD0748+436 See also (NC) WD0749+426 See also (PV)(OJ) WD0750+267 See also (NC) WD0750+317 See also (NC) WD0750+379 See also (NC) WD0751+299 See also (NC) WD0751-252 See also (OJ) WD0751-595 Foreground star not a cluster member, Ref.(8S). WD0752+278 See also (NC) WD0752+398 DA with very noisy spectrum; Ref.(QB)See also (NC) WD0752+402 See also (MS)(NR) WD0752+424 See also (NC) WD0752+492 Double-degenerate merger system. Ref.(QT). WD0752-146 Slight variability in radial velocity indicates a possible binary. Emission line has a VR0= -146.8km/s. (EE) See also (QP) WD0752-676 See also (OL)(OJ)(RQ) WD0753+313 See also (NC) WD0753+478 See also (NC) WD0753+535 VV47 is a PG1159 star with no detected variability and an associated planetary nebula, Ref.(5O)(1M); type E, Ref.(66). WD0754+326 See also (QJ)(NC) WD0754+402 See also (OK) WD0755+358 See also (PD)(MV) WD0756+324 See also (NC) WD0756+350 See also (NC) WD0756+437 A new magnetic degenerate with a 220 MG field, Ref.(8N). WD0756+493 See also (NC) WD0756-607 Foreground star not a cluster member, Ref.(8S). WD0757+075 See also (QJ) WD0757+118 See also (QJ) WD0757+501 See also (NC) WD0757-603 Member of the open cluster NGC 2516, Ref.(8S). WD0757-606.1 Member of the open cluster NGC 2516, Ref.(8S). WD0757-606.2 Member of the open cluster NGC 2516, Ref.(8S). WD0758+224 See also (NC) WD0758-476 See also (JV) WD0800+233 See also (NC) WD0800+417 See also (NC) WD0801+186 See also (PD)(MV) WD0801-608 Foreground star not a cluster member, Ref.(8S). WD0802+220 See also (PD)(MV) WD0802+386 See also (OR) WD0803+340 See also (NC) WD0803+407 See also (NC) WD0804+075 See also (QJ)(NC) WD0804+397 See also (MV) WD0805+185 See also (QJ) WD0805+654 See also (JV) WD0806+312 See also (RS) WD0806+376.1 See also (PD)(MV) WD0806-661 L0097-003 shows strong UV CI absorption, Ref.(DD) See also (OJ). WD0807+190 Probably a moderate velocity red dwarf. private comm. J.Farihi 9/2008 WD0807+416 See also (NC) WD0807+463 Reclassified as M star; Ref.(QB)See also (NC) WD0807+484 See also (PR) WD0808+058 See also (QJ)(NC) WD0808+272 See also (MT) WD0809+034 See also (NC) WD0809+235 See also (NC) WD0810+234 See also (PQ) WD0810+329 See also (NC) WD0810+455 See also (NC) WD0810+489 See also (OJ) WD0810-728 See also (PP)(RK) WD0811+111 WD+MS Eclipsing Binary System. Ref.(QN). WD0811+411 See also (NC) WD0811+414 See also (NC) WD0812+208 See also (QJ) WD0812+433 See also (NC) WD0812+436 WD/MS binary nature questionable. Ref.(QB) WD0812+447 ZZ Ceti star Ref.(KB) WD0812+478 Name(s) for MS companion(s). PG 0812+478B WD0813+265 See also (NC) WD0813+358 See also (NC) WD0814+001 See also (QJ) WD0814+043 See also (PD)(MV) WD0814+058 See also (QJ)(NC) WD0814+271 See also (NC) WD0815+176 See also (QJ) WD0815+357 Double-degenerate merger system. Ref.(QT)(QS). WD0816+356 See also (NC) WD0816+376 GD90 magnetic, not polarized, Zeeman H lines, Ref.(05)(03). WD0816+433 Post-common envelope binary. Ref.(QB)See also (QJ)(NC) WD0816-310.1 See also (OJ) WD0817+062 See also (QJ)(NC) WD0817+255 See also (NC) WD0818+461 See also (NC) WD0819+280 Double-degenerate merger system. Ref.(QT)(SL). WD0819+355 See also (NC) WD0819+461 See also (NC) WD0820+250.1 See also (PM) WD0821+175 See also (QJ) WD0821+275 See also (NC) WD0821-252 See also (RK)(OQ)(MV) WD0821-669 See also (PV)(OJ) WD0822+036 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD0822+342 See also (NC) WD0822+414 ZZ Ceti star Ref.(KB) WD0823+039 See also (NC) WD0823+062 DA; binary nature questionable. Ref.(QB)See also (NC) WD0823+316 Central star of PN. Ref.(QM) See also (QP) WD0823+336 See also (NC) WD0824+066 DA; binary nature questionable. Ref.(QB)See also (NC) WD0824+082 Reclassified as M star; Ref.(QB)See also (NC) WD0824+288 Double lined spectroscopic binary, DA + dwarf carbon star, Ref.(2R). dC companion VR0 = -36.8(EE) Triple system: DA+dC+M3V (IH)(JV), see A5.4 Ref.(LJ) See also (QO)(QP) WD0824+474 See also (NC) WD0825+072 DA; binary nature questionable. Ref.(QB)See also (NC) WD0825+297 See also (PD)(MV) WD0826+271 See also (NC) WD0826+282 DA binary nature questionable. Ref.(QB)See also (NC) WD0827+080 Reclassified as M star; Ref.(QB) WD0827+291 See also (NC) WD0827+321 See also (NC) WD0827+368 DA; binary nature questionable Ref.(QB)See also (NC) WD0827+410 See also (RY) WD0827+472 See also (NC) WD0828+081 Reclassified as MS + bright star; Ref.(QB) WD0828+412 See also (NC) WD0830+536 See also (NC) WD0830-535 See also (PP)(NO)(RK) WD0831+056 See also (NC) WD0831+072 See also (QJ)(NC) WD0831+140 See also (QJ) WD0832+436 See also (NC) WD0833+049 Cataclysmic variable? Ref.(QB)See also (QJ)(NC) WD0833+198 See also (OS) WD0834+087 Reclassified as M star + star nearby; Ref.(QB) WD0834+270 See also (NC) WD0834+500 See also (JE) WD0834+532 See also (NC) WD0835+194 WD+MS Eclipsing Binary System. Ref.(QN). WD0836+197 Praesepe member. See also (OS) WD0836+199 Praesepe member. See also (OS) WD0836+201 Praesepe member. See also (OS) WD0836+237 See also (NL) WD0836+404 ZZ Ceti star ref.(KA) WD0837+189 See also (OS) WD0837+199 Praesepe member. See also (OS)(MV) WD0837+218 See also (OS) WD0837+271 See also (NC) WD0837+273 See also (MV) WD0837+280 See also (NC) WD0837+283 See also (NC) WD0837+330 See also (MS) WD0837+458 See also (NC) WD0838+035 See also (JV) WD0838+375 CBS78 is the second known DB star showing accreted calicium, Ref.(AN).See also (RS) WD0839+025 See also (PD)(MV) WD0839+086 See also (NC) WD0839+179 MS+MS superposition; Ref.(QB) WD0839+345 See also (OK) WD0839+372 ZZ Ceti star Ref.(KB) WD0839-327 See also (PV)(PP)(PC)(OJ)(MV)(MM)(NB)(NL)(OL)(RQ) WD0839-528 Not a confirmed cluster member, Ref.(4O)(JV). WD0840+047 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD0840+126 See also (QJ) WD0840+190 See also (OS) WD0840+200 Possible PRAESEPE member, Ref.(BV)(JV). See also (OS) WD0840+209 See also (OS) WD0840-136 See also (OJ) WD0841+055 See also (NC) WD0841+098 See also (NC) WD0841+218 DA; binary nature questionable. Ref.(QB) WD0842+375 See also (NC) WD0842+490 See also (JV) WD0843+058 DA; binary nature questionable. Ref.(QB) WD0843+186 See also (OS) WD0843+358 See also (OJ) WD0843+488 Possible unresolved DA/DC spectroscopic binary. Ref.(PD) WD0844+287 See also (NC) WD0844+453 ZZ Ceti star Ref.(KB) See also (NQ) WD0845+011 See also (QJ)(NC) WD0845+440 See also (NC) WD0845-188 CPMB WITH CD-18 2482 See also (PR) WD0846+006 See also (RF)(RS) WD0846+049 Double-degenerate merger system. Ref.(QT). WD0846+052 See also (QJ)(NC) WD0846+081 DA; binary nature questionable.Ref.(QB) WD0846+249 See also (JE) WD0846+346 See also (QA)(MR)(OH)(RY) WD0847+456 See also (NC) WD0848+007 See also (QJ)(NC) WD0848+037 See also (QJ)(NC) WD0848+062 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD0849+049 Possible double-degenerate system. Ref.(SL) WD0849+068 See also (NC) WD0849+276 See also (QJ) WD0849+319 See also (QX) WD0849+549 See also (NC) WD0850+472 See also (NC) WD0850-617 (P.Bergeron Finding Chart) WD0853+049 See also (QJ)(NC) WD0853+057 See also (NC) WD0853+069 See also (NC) WD0853+163 Misidentified as LB 8827 in much of the literature (IW) WD0854+158 See also (QJ) WD0855+039 WD+MS Eclipsing Binary System. Ref.(QN). WD0855+328 See also (NC) WD0855+373 See also (NC) WD0855+407 See also (NC) WD0855+416 See also (PD)(MV) WD0855+583 See also (NC) WD0855+604.1 See also (PR) WD0855+604.2 Possible CV? Ref.(AT). See also (PR) WD0856+047 See also (QJ)(NC) WD0856+331 EG182 common proper motion binary with HD77408 (F8 dwarf); G47-18 is a strong carbon band, DQ star polarized, Ref.(75). Section A2.1 in Ref(LJ) reports different motions for the pair therefore not CPMB. See also (OJ) WD0856+577 See also (RS) WD0857+001 See also (OY) WD0857+086 See also (QJ) WD0858+363 GD99 is a ZZ CETI variable, Ref.(7M) See also (PB)(NL) WD0858+441 DA; binary nature questionable.Ref.(QB)See also (NC) WD0859+337 See also (OK) WD0859+391 Reclassified as carbon star; Ref.(QB) WD0859-039 See also (MV) WD0900+426 See also (NC) WD0900+565 See also (NC) WD0901+016 See also (OY) WD0901+140 Visual double degenerate Finding chart for PG 0901+140B see A5.8 in Ref.(LJ) WD0901+530 See also (OY) WD0902+060 See also (QJ) WD0902+097 See also (QJ)(NC) WD0903+083 Possible unresolved DA/DC spectroscopic binary. Ref.(PD) See also (MV) WD0903+166 See also (JV) WD0903-002 ZZ Ceti star Ref.(KB) WD0904+358 See also (PD)(MV) WD0904+511 See also (JV) WD0905+062 WD/MS eclipsing binary system. Ref.(PH) See also (QJ)(NC)(QH)(QN) WD0905+372 See also (NC) WD0905+538 See also (QJ)(NC) WD0905-724 See also (SM) WD0906+006 See also (RF)(RS) WD0906+076 See also (NC) WD0906+296 See also (PR) WD0908+033 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD0908+171 See also (PP) WD0908+226 DA star, spectroscopic composite with dM(LP369-15B), Ref.(7Z). See also (QJ) WD0908+422 See also (PD)(MV) WD0910+014 See also (QJ)(NC) WD0910+584 See also (MS) WD0910+593 See also (NC) WD0911+059 See also (PD)(MV) WD0911+651 See also (PR) WD0912+105 See also (NC) WD0912+318 See also (NC) WD0912+453 See also (NC) WD0912+536 Polarization observed, Ref.(06) See also (PV)(PO)(OL)(MV)(NB)(NN)(OJ)(RQ) WD0913+055 Propose that spectrum originates from two unrelated stars on same line of sight. Ref.(MS) WD0913+408 See also (NC) WD0913+442 EG64 common proper motion binary with G115-64 (G5 dwarf), Ref.(75). Section A2.1 in Ref(LJ) reports different motions for the pair therfore not CPMB See also (NZ)(PQ) WD0913+444 See also (NC) WD0913-003 See also (QJ)(NC) WD0914+096 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD0914+610 See also (NC) WD0914-195 See also (OQ)(JV)(RK) WD0915+180 See also (QJ) WD0915+201 Name(s) for MS companion(s). LB 3016B WD0915+414 See also (NC) WD0915+551 See also (NC) WD0916+064 See also (OK) WD0916+090 See also (NC) WD0917+430 See also (NC) WD0917-000 See also (NC) WD0918+047 See also (NC) WD0918+111 See also (NC) WD0918+398 See also (NC) WD0918+593 DA; binary nature questionable.Ref.(QB)See also (NC) WD0919+003 See also (OY) WD0919+104 See also (NC) WD0920+015 ZZ Ceti star Ref.(KB) WD0920+306 Double-degenerate merger system. Ref.(QT). WD0921+012 See also (NC) WD0921+016 See also (QJ)(NC) WD0921+020 See also (NC) WD0921+354 G117-B15A is a ZZ CETI variable, Ref.(7M) See also (PB)(8W)(JE)(NL)(PQ) WD0922+006 See also (QJ)(NC)(QH) WD0922+014 See also (PD)(MV) WD0922+065 See also (NC) WD0922+162 Double degenerate ref.(JE) See also (PP) WD0922-000 See also (QJ)(NC) WD0923+219 See also (QJ) WD0924+337 See also (NC) WD0925+386 See also (NC) WD0925+498 DA; binary nature questionable.Ref.(QB) WD0926+084 Hot/cold Table 1 temperatures ambigious. Ref.(PP) WD0928+379 See also (NC) WD0928+399 See also (NC) WD0928+399.1 See also (NC) WD0928-713 Additional updated chart by P.Bergeron 3/20/07 - Click T.R.Marsh Chart WD0929+350 See also (NC) WD0929+380 DA?; binary nature questionable. Ref.(QB) See also (QM) WD0930+096 See also (NC) WD0930+294 See also (MY) WD0930+815 A DA white dwarf companion to the hybrid K3II giant HD81817A See also (SM) WD0931+034 See also (QJ)(NC) WD0931+054 See also (QJ)(NC) WD0931+058 See also (NC) WD0931+105 See also (PD)(MV) WD0931+444 See also (NC) WD0931+507 See also (PD)(MV) WD0932+230 WD+MS Eclipsing Binary System. Ref.(QN). WD0933+025 Name(s) for MS companion(s). PG 0933+025B WD0933+345 See also (NC) WD0933+423 See also (NC) WD0933+526 Spectrum shows Mg I, Ref.(JJ) WD0933+729 Possible companion Finding chart for PG 0933+729B see A4.3 in Ref.(LJ) WD0934+020 See also (RF)(RS) WD0934+067 See also (NC) WD0934-587 (P.Bergeron Finding Chart) WD0935+577 See also (NC) WD0935-371.1 Strong UV CI lines, Ref.(CK) See also (PR). WD0935-371.2 Very close white dwarf pair; UBV photometry, Ref.(61) See also (PR). WD0936+054 See also (QJ)(NC) WD0936+331 WD+MS Eclipsing Binary System. Ref.(QN). WD0936+378 See also (NC) WD0936+382 See also (NC) WD0936+560 See also (RF)(RS) WD0936+563 ZZ Ceti star Ref.(KB) WD0936+595 See also (NC) WD0937+049 DA; binary nature questionable.Ref.(QB)See also (NC) WD0937+505 See also (JV)(MZ)(NO)(OK)(RK) WD0937+513 See also (NC) WD0937+527 See also (NC) WD0938+002 See also (NC) WD0938+065.1 See also (QJ) WD0938+550.1 See also (PM) WD0938+577 ZZ Ceti star Ref.(KB) WD0939+071 Spectra doesn't look like a single WD, P.Bergeron and J.Holberg, private comm 3/2008. See also (PS)(OJ) WD0939+262 See also (QP)(NL) WD0940+114 Hot/cold Table 1 temperatures ambigious. Ref.(PP) WD0940+608 Possible sdOB/WD binary system. Ref.(QX). WD0940+619 See also (QJ)(NC) WD0941+432 See also (OK) WD0941+458 See also (PD)(MV) WD0942+236.1 See also (PR) WD0942+236.2 See also (PR) WD0943+441 See also (QP)(NL) WD0944+115 See also (NC) WD0944+424 See also (RY) WD0944+452 has a common proper motion WD companion 20" away Ref.(KR)(OM) WD0945+021 See also (OY) WD0945+127 See also (NC) WD0945+245 LB11146 is a magnetic DX degenerate in a double degenerate binary with a non-magnetic DA companion, Ref.(5I) See also (QP)(JE)(MV). WD0945+372 See also (NC) WD0945+578 See also (QJ)(NC) WD0946+002 ZZ Ceti star Ref.(KB) WD0946+020 See also (NC) WD0946+036 See also (QJ)(NC) WD0946+488 See also (NC) WD0946+534 See also (OJ) WD0947+016 See also (NC) WD0947+452.1 CPMB with WD 0947+452 Ref.(QL). WD0947+857 See also (NL)(RK) WD0948+031 See also (QJ)(NC) WD0948+043 See also (QJ)(NC) WD0949+256 Double degenerate ref.(JE) WD0949+451 Resolved triple (WD+dM4.5+dM4.5) system. Ref.(MQ) See also (QP) WD0949+484 See also (NC) WD0949+495 See also (OK) WD0950+021 See also (OY)(MT) WD0950+023 See also (OK) WD0950+139 DA star with Teff > 1E+5K, Planetary Nebula nucleus, Ref.(5P). WD0950-200 Double degenerate close binary, Ref.(45). WD0951+132 ZZ Ceti star Ref.(KB) WD0951+442 See also (OY) WD0952+094 Reclassified as carbon star; Ref.(QB)See also (NC)(MV) WD0952+182 ZZ Ceti star Ref.(KB) WD0953+594 See also (RF)(RS) WD0953+621 See also (NC) WD0954+007 DA; binary nature questionable.Ref.(QB)See also (NC) WD0954+013 See also (OY) WD0954+023 See also (NC) WD0954+239 WD+MS Eclipsing Binary System. Ref.(QN). WD0954+247 This star is listed in ref.(EE) as being a white dwarf. WD0954+342 SW LMI is a non-radial pulsator, Ref.(44). WD0954+697 See also (JV) WD0954-710 See also (NL) WD0955+017 ZZ Ceti star Ref.(KB) See also (NQ) WD0955+247 See also (PP)(OJ) WD0955+412 See also (NC) WD0956+045 Visual double see A5.20 in Ref.(LJ) See also (PS)(PP) WD0957+022 See also (PD)(MV) WD0957+028.1 See also (NC) WD0957+089 See also (NC) WD0957+112 See also (NC) WD0957-666 Possible double degenerate binary, Ref.(BY) See also (MV). WD0958+024 See also (NC) WD0958+102 See also (NC) WD0959+038 See also (NC) WD0959+441 See also (NC) WD1000+044 See also (NC) WD1000+220 Probably Late A or early F star Ref.(PS) WD1000-001 See also (PP)(OK) WD1001+058 See also (PD)(MV) WD1001+203 Name(s) for MS companion(s). Ton1150B See also (QP) WD1001+473 See also (NC) WD1002+525 See also (NC) WD1003+009 See also (QJ)(NC) WD1003+230 WD+MS Eclipsing Binary System. Ref.(QN). WD1003+612 See also (NC) WD1003-441 LONGMORE 4 is a PG1159 star with 9-11 detected periods and an associated planetary nebula mass ejection, Ref.(DJ); type lgEp, Ref.(66) Non-radial g-mode pulsator Ref.(KO)N. WD1004+124 See also (NC) WD1004+128 See also (PD)(MV) WD1004+409 See also (NC) WD1005+002 ZZ Ceti candidate (HC) WD1005+465 See also (NC) WD1006+029 See also (QJ)(NC) WD1006+431 Superposition of three stars; Ref.(QB) WD1007-002 See also (QJ)(NC) WD1008+053 See also (OY) WD1008-179 NOTE: Should be classified as an extremely hot, Teff > 100,000K, from ref(LX). WD1009+034 See also (NC) WD1009-184 Wide CPMB with the K7V star LHS 2231. Ref.(OJ) See also (RZ) WD1010+043 See also (OK) WD1010+049 See also (NC) WD1010+049.1 See also (NC) WD1010+064 See also (JV)(NL)(OK) WD1011+459 See also (NC) WD1011+470 See also (OY) WD1011+601 ZZ Ceti star Ref.(KB) See also (NQ) WD1012+093 See also (PD)(MV) WD1013+033 ZZ Ceti star Ref.(KB) WD1013+044 See also (PD)(MV) WD1013+494 See also (NC) WD1013-010 Single-lined double-degenerate binary. Ref.(PP) WD1013-050 DAO white dwarf in a pre-CV, RE1016+053, REF.(BC), Quadruple system DAO + 3 dM stars, Ref(LJ) See also (QH)(MV)(RK) WD1014+083 See also (NC) WD1014-009 See also (QJ) WD1015+014 Polarized magnetic white dwarf, Ref. (04) See also (PD)(MV) WD1015+076 Finding chart for PG 1015+076B see A5.21 in Ref.(LJ) WD1015+161 See also (QV)(QD)(QA)(PP)(OR)(MR) WD1015+468 See also (NC) WD1015-173 Name(s) for MS companion(s). EC 10150-1722B WD1015-216 See also (PP) WD1016+406 See also (NC) WD1016+535 See also (NC) WD1016-044 See also (QV) WD1017+125 Finding chart for PG 1017+125B Ref.(LJ) WD1017+366 GD116 is a magnetic degenerate, Ref.(9L). WD1017-138 See also (PP) WD1018+515 See also (NC) WD1019+462 Binary (WD+M0) system. Ref.(MK) See also (PR) WD1019+583 See also (NC) WD1019+637 See also (OJ) WD1020+047 See also (NC) WD1020+442 See also (NC) WD1020+541 See also (MS)(NR) WD1022+009 See also (NN) WD1022+050 Double-degenerate candidate Ref.(KP). See also (QX) WD1022+108 See also (NC) WD1022-301 See also (RK)(OQ) WD1023+009 See also (PP)(OK) WD1023+305 See also (QJ) WD1024-002 ZZ Ceti candidate (HC) WD1026+002 Radial Velocities 36.5/48.0 km/sec Ref.(JP) Section A3.2 in Ref.(LJ) indicates the companion is a high velocity background star, not a CPMB See also (QX)(QX)(QP)(MY)(NL) WD1026+023 PCEB. Ref.(QH)(SM). WD1026+117 LHS2273 is a magnetic degenerate, Ref.(28) See also (MV) WD1026+453 See also (NL)(OK)(RK) WD1027+398 See also (NC) WD1027+469 See also (NC) WD1029+537 See also (QM)(JV) WD1030+598 See also (NC) WD1031+063 See also (PP) WD1031+234 A new magnetic degenerate with a field strength exceeding 500 megagauss, Ref.(9Y)(JE)N. WD1031-114 See also (PP)(NB)(NL)(RK) WD1032+027 See also (NC) WD1032+109 See also (NC) WD1032+216 Possible unresolved DA/DC spectroscopic binary. Ref.(PD) WD1032+393 See also (NC) WD1032+400 Reclassified as carbon star; Ref.(QB)See also (NC) WD1033+464 Composite spectrum with dM(GD 123B), Ref.(9V), also see Section A5.14 in Ref.(LJ) See also (QP)(NL) WD1033+656 See also (MV) WD1033+714 See also (OJ) WD1034+001 Hot DO degenerate with C,N,O,Si absorption in the far UV, Ref.(AL) See also (RN) WD1034+074 See also (RS) WD1034+077 LHS2288 MV > 15.0, Ref.(51). WD1034+492 See also (OK) WD1034+661 See also (NC) WD1036+021 Peculiar secondary star. Ref.(QB) WD1036+085 See also (OK) WD1036-204 LP790-29 is a polarized,carbon band,magnetic degenerate, Ref.(5G) See also (PS)(OJ). WD1037+256 See also (QJ) WD1037+512 Name(s) for MS companion(s). PG 1037+512B WD1037+521 See also (NC) WD1038+088 See also (QJ)(NC) WD1038+096 See also (NC) WD1038+518 See also (NC) WD1038+633 See also (OK) WD1039+447 See also (NC) WD1040+054 See also (NC) WD1040+406 See also (NC) WD1040+421 See also (OY) WD1040+451 See also (JV)(OK) WD1040+492 See also (QM) WD1041+063 See also (QJ)(NC) WD1041+091 See also (QD)(OR) WD1041+580 See also (QP)(NL)(NO) WD1042+322 See also (PE) WD1042-000 See also (QJ)(NC) WD1042-690 PCEB DAQZ + dM5 Ref.(RV).See also (QH)(PP)(MV) WD1043+600 See also (NC) WD1043+610 See also (NC) WD1043-034 CPMB system with the F9 V star G163-B9A. Ref.(OF) WD1043-188 See also (OJ)(NN)(PR) WD1045+056 PCEB Ref.(QH).See also (QJ)(NC) WD1045+629 See also (NC) WD1045-091 HE1045-0908:a new magnetic DA white dwarf with a distinctive Zeeman line splitting pattern, Ref.(8R). WD1046+398 See also (NC) WD1047-046 See also (QX) WD1048+668 See also (NC) WD1049+103 Name(s) for MS companion(s). PG 1049+103B WD1049+266 See also (QJ) WD1050+522 Double-degenerate merger system. Ref.(QT).See also (QS)(SL) WD1050+541 Reclassified as M star; Ref.(QB)See also (NC) WD1050+598 See also (PD)(MV) WD1051+516 Name(s) for MS companion(s). SBS 1051+516B See also (QP) WD1051+533.1 CPMB with WD1051+533.2 WD1051+533.2 CPMB with WD1051+533.1 WD1052+273 See also (QP)(MY)(NL) WD1053+001 ZZ Ceti star Ref.(KB) WD1053+017 See also (RF)(RS) WD1053+049 See also (NC) WD1053+511 See also (NC) WD1053+656 See also (PD)(MV) WD1053-092 See also (PP) WD1053-290 See also (PP) WD1053-550 Additional updated chart by P.Bergeron 3/20/07 - Click T.R.Marsh Chart See also (MV) WD1054+501 Reclassified as M star; Ref.(QB) WD1055-072 DA6 observed to be featureless? Ref.(9V)(NB)(NN) See also (PV)(PO)(OL)(OJ)(RQ). WD1056+012 See also (NC) WD1056+516 DA1 may be a double degenerate, Ref.(81)(JV) See also (OK)(RK) WD1056+559 See also (OY) WD1056-384 See also (PP)(RK) WD1057+719 See also (QP)(NL)(RK) WD1058+078 See also (NC) WD1058+140 See also (QJ) WD1058-129 See also (PP) WD1059+126 See also (QJ)(NC) WD1059+559 Relcassified as M star + bright star nearby; Ref.(QB) WD1101+364 double degenerate DA + DA double lined, Ref.(7F). See also (QX) WD1102+095 Single-lined double-degenerate binary. Ref.(PP) WD1102+253 Detached magnetic cataclysmic variable. Ref.(QB) WD1102+748 See also (MY) WD1102-183 See also (QA)(PP)(OH) WD1103+015 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD1103+078 See also (NC) WD1103-008 See also (NC) WD1104+602 See also (QP)(NL) WD1104+656 See also (NC) WD1105+053 See also (NC) WD1105+097 See also (NC) WD1105+412 See also (PR) WD1105-048 See also (JE)(MZ)(NL)(PR) WD1105-340 CPMB with M4Ve companion Ref.(MD) WD1106+121 See also (NC) WD1106+316 Name(s) for MS companion(s). Ton 058B WD1107+055 Reclassified as MS+galaxy; Ref(.QB)See also (NC) WD1107+310 Wide-binary? Ref.(QB) WD1107+602 See also (PD)(MV) WD1107-257 Common proper motion pair. See also (PR) WD1108+207 See also (NN) WD1108+325 Name(s) for MS companion(s). Ton 060B See also (QP) WD1108+563 See also (OK) WD1109+244 See also (JV)(NL) WD1109-005 ZZ Ceti candidate (HC) WD1111+455 See also (NC) WD1112+096 See also (QJ)(NC) WD1112+432 Reclassified as CV; Ref. QB) WD1112+669 See also (NC) WD1113+542 See also (NC) WD1114+026 See also (NC) WD1114+113 See also (QJ)(NC) WD1115+017 See also (QJ)(NC) WD1115+101 See also (PD)(MV) WD1115+135 See also (QJ)(NC) WD1115+158 A new pulsating DB star, Ref.(DV). WD1115+166 An Unresolved DAB Double Degenerate Binary. (GW)(HE)(JE)N See also (QX)(QX) WD1116+026 ZZ Ceti (OD)See also (QV)(QD)(QA)(PP)(OR)(MR)(NL) WD1116+301 See also (QX) WD1116-470 See also (PV) WD1119+042 ZZ Ceti star Ref.(KB) WD1120+008 See also (QJ)(NC) WD1120+102 Possible unresolved DA/DC spectroscopic binary. Ref.(PD) WD1120+439 See also (MY) WD1120+509 Spectrum shows Mg I, Ref.(JJ) WD1121+216 Ross 627 is a DA white dwarf not DA, F or DF, Ref.(6A) See also (PV)(PO)(OL)(MM)(NB)(NN)(OJ)(RQ) WD1121-008 See also (NC) WD1122+546 See also (OK) WD1123+014 See also (QJ)(NC) WD1123+040 ZZ Ceti star Ref.(KB) See also (NQ) WD1123+056 MS+MS superposition Ref.(QB) WD1123+189 Composite DA + DM binary, Ref.(9V) See also (QP)(MY)(NL) WD1124+152 See also (QJ) WD1124+431 See also (NC) WD1124-018 Single-lined double-degenerate binary. Ref.(PP) WD1124-293 See also (QV)(QA)(OH) WD1125+131 See also (NC) WD1125-002 See also (QJ)(NC) WD1126+089 See also (NC) WD1126+185 See section A1.3 in Ref. (LJ). WD1126+499 NOTE: 2000 coords are from ref(MH),Ref(LR) gives J112924.74+493931.9 but no star found at these coords using SDSS Finding Chart Tool. See also (PD)(MV) WD1126+668 See also (QJ)(NC) WD1126-008 See also (PD)(MV) WD1127+319 See also (PE) WD1129+071 See also (PP) WD1129+284 Possible unresolved DA/DC spectroscopic binary. Ref.(PD) WD1129-030 See also (QJ)(NC) WD1131+521 See also (PD)(MV) WD1132+661 See also (QJ)(NC) WD1132-298 (P.Bergeron Finding Chart) WD1132-325 Sirius-like system. Ref.(RZ) See also (OJ) WD1133+358 Name(s) for MS companion(s). G147-065B WD1133+489 Name(s) for MS companion(s). PG1133+489B See also (QP) WD1134+044 See also (QJ)(NC) WD1134+300 No 1400a absorption feature observed, Ref.(CL)(JV) See also (QP)(MY)(NB)(NL)(OJ) WD1135+000 See also (NC) WD1135+579 Possible unresolved DA/DC spectroscopic binary. Ref.(PD) See also (MV) WD1136+514 See also (NC) WD1136-015 LBQS1136-0132 is a magnetic degenerate, Ref.(85) See also (PD)(MV) WD1137+423 ZZ Ceti star ref.(KA) See also (RY) WD1137+582 Reclassified as M star + bright star nearby; Ref.(QB) WD1137+614 See also (MV) WD1138+046 See also (NC) WD1138-026 See also (NC) WD1140+004 ZZ Ceti candidate (HC) PCEB. Ref.(QH). See also (QP)(QJ)(PS)(NC) WD1141+462 See also (NC) WD1141+504 See also (NC) WD1142+385 Cataclysmic variable? Ref.(QB) WD1142-645 L0145-141 shows strong UV absorption features, Ref.(DC) Member of binary or multiple star system. Ref.(OJ) See also (PC)(OE). WD1143+321 See also (QP)(NL)(1P)(AP) WD1144+004 PG1159 degenerate, Ref.(DI); type EP, Ref.(66)(JV) See also (RN) WD1144+016 MS+MS superposition; Ref.(QB) WD1144+299 See also (PE) WD1144-246 See also (PP) WD1145+041 See also (QJ)(NC) WD1145+187 See also (QP)(PP) WD1145+487 See also (PD)(MV) WD1146+443 See also (NC) WD1146-015 See also (NC) WD1147+255 Common proper motion binary Ref.(JP) See also (PP)(PQ)(PR) WD1147-010 See also (NC) WD1148+544 LP129-587 is a CPMB with LP129-586 Ref.(JL) See also (OK) WD1148-230 = EC11481-2303 See also (NF) WD1149+001 Irradiated secondary star. Ref.(QB)See also (QJ)(NC) WD1149+057 ZZ Ceti (OC) See also (PP) WD1149+280 See also (PE) WD1150+006 See also (NC) WD1150-153 Short period ZZ Ceti (OC) See also (QD)(QA)(OR) WD1151+015 See also (PD)(MV) WD1151+548 See also (NC) WD1151-029 PG1159 degenerate, Ref.(DN); type LGE, Ref.(66). WD1152-000 See also (RS) WD1154+061 ZZ Ceti star Ref.(KB) WD1154+456 DB; binary nature questionable. Ref.(QB) See also (QM) WD1155+492 See also (QX) WD1156+117 See also (NC) WD1156+129 Name(s) for MS companion(s). WD 1156+129B WD1156+132 See also (PS) WD1156+619 See also (PD)(MV) WD1158-362 See also (RK) WD1159+619 See also (PD)(MV) WD1159+803 G255-002 is a ZZ CETI variable, Ref.(BN). See also (PB) WD1159-034 Proto-type of a new class of pulsating, hot, helium-rich DO degenerates (PG1159), Ref.(7K); type E, Ref.(66)(JV) Non-radial g-mode pulsator Ref.(KO) See also (RN) WD1200+548 See also (OK) WD1201+035 See also (QJ)(NC) WD1201-001 See also (PP)(MZ) WD1201-023 ZZ Ceti candidate (HC) WD1202+034 See also (QJ)(NC) WD1202+608 Peculiar DAO white dwarf in a pre-CV; binary? Ref.(29), close double degenerate Ref.(3L)(JE)N. See also (QX) WD1202-232 See also (QV)(PP)(OJ)(OL)(RQ) WD1203+085 See also (PD)(MV) WD1203+097 See also (NC) WD1203+432 See also (QJ)(NC) WD1204+444 See also (PD)(MV) WD1204+450 Triple system Finding chart for PG 1204+450C see A5.5 in Ref.(LJ) WD1204-026 ZZ Ceti candidate (HC) WD1204-136 See also (QA)(OH) WD1206+654 See also (NC) WD1207-005 See also (QJ)(NC) WD1207-157 See also (PP) WD1208+039 See also (NC) WD1208+422 See also (NC) WD1208+576 See also (OJ)(OH) WD1208-025 See also (QJ)(NC) WD1209+018 Magnetic DA+L brown dwarf; Ref.(QB)See also (PD)(NC)(MV) WD1210+140 Single-lined double-degenerate binary. Ref.(PP) See also (QP) WD1210+464 Name(s) for MS companion(s). PG 1210+464B See also (QP) WD1210+533 Peculiar DAO white dwarf, Ref.(3M)(JE),Spectroscopic Variable,Ref(QM). WD1210-011 WD/MS eclipsing binary system. Ref.(PH) PCEB(SD) See also (NC)(QH)(QN) WD1210-060 CMPB with the K3V star HIP 59519. Ref.(SH) WD1211+332 See also (QP) WD1211+392 See also (PR) WD1211-025 MS+MS superposition; Ref.(QB)See also (NC) WD1211-169 HS1211-170 is a new magnetic degenerate, Ref.(4C). WD1212+369 See also (QH) WD1212+589 See also (NC) WD1212-022 Heavily blanketed, cool(~6000K) magnetic(Zeeman split NaI and MgI) DZ. (EM) WD1213+096 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD1213+437 See also (NC) WD1213+528 DA and dwarf M spectroscopic binary post-common envelope, Ref.(5A); DA degenerate with T=13,000K; log g=8; 1400A absorption, Ref.(AQ)(JV). See also (QX)(SM) WD1213+532 DA; binary nature questionable. Ref.(QB) See also (QM) WD1214+032 Companion = LP554-064 with Vmag=13.28 See also (PR) WD1214+267 See also (JE) WD1214-001 See also (PD) WD1215+009 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD1215+024 See also (OK) WD1215+323 See also (PR) WD1216+036 See also (PP) WD1217+475 DC; binary nature questionable. Ref.(QB) WD1217+635 See also (NC) WD1218+496 See also (NC) WD1218+497 Name(s) for MS companion(s). PG 1218+497B See also (QP) WD1219+005 See also (PD)(MV) WD1219+098 See also (NC) WD1219-024 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD1220+234 PG1220+234 is a magnetic degenerate, Ref.(31) See also (MV) WD1220+441 See also (OY) WD1220+484 See also (PD)(MV) WD1220-003 See also (OY) WD1221+422 See also (PD)(MV) WD1221-006 See also (QJ)(NC) WD1223-659 See also (OJ)(MM)(OL)(RQ) (P.Bergeron Finding Chart) WD1224+309 PCEP(QH) See also (QJ) WD1225+006 See also (QV)(QA) WD1225+589 DA; binary nature questionable.Ref.(QB) See also (QM) WD1225+637 Spectrum shows Mg I, Ref.(JJ) WD1225-015 See also (NC) WD1225-079 See also (PS)(OR) WD1226+109 See also (QD)(QA)(OR) WD1227+292 See also (PR) WD1228+541 See also (NC) WD1229+290 See also (JV) WD1229+558 See also (QJ)(NC) WD1229-028 See also (QJ)(NC) WD1230+163 Double-degenerate merger system. Ref.(QT). WD1230+596 See also (NC) WD1230+605 See also (NC) WD1231+130 DA; binary nature questionable.Ref.(QB)See also (PD)(NC)(MV) WD1231+447 See also (NC) WD1231-021 Double-degenerate merger system. Ref.(QT). WD1232+065 See also (QJ) WD1234+481 Hot DA and a very low-mass detached companion. Ref.(RO).See also (QP)(JV)(NB)(NL)(SM) WD1235+012 DA; binary nature questionable.Ref.(QB)See also (NC) WD1235+294 Coordinates in ref (BV) are incorrect, Private Communication 4/24/2011 P.Bergeron WD1235+620 See also (NC) WD1236+012 See also (NC) WD1236+457 Listed in ref (NN) as WD1239+454 WD1236+661 See also (NC) WD1236-004 Name(s) for MS companion(s). WD 1236-004B See also (QP) WD1236-495 BPM 37093 is a ZZ CETI variable, Ref.(44) See also (PP)(PB)(MY)(NB)(NL)(OJ) WD1237+487 See also (NC) WD1237-028 See also (MY) WD1238+439 See also (NC) WD1238+618 See also (NC) WD1239+143 See also (QJ) WD1239+277 See also (RY) WD1240+453 See also (NC) WD1240+644 See also (NC) WD1241+151 See also (QJ) WD1241+235 See also (PP) WD1241+483 See also (OK) WD1241-010 New double degenerate close binary, Ref.(7G), Triple system, see section A5.6 in Ref.(LJ). See also (QX)(PP)(RO) WD1242+105 WD+MS Eclipsing Binary System. Ref.(QN). WD1242-105 See also (OJ) WD1244+149 See also (PQ) WD1244+498 See also (RS) WD1244-125 See also (PP) WD1245+413 Possible unresolved DA/DC spectroscopic binary. Ref.(PD)See also (MV) WD1246+441 See also (NC) WD1246-022 See also (PD)(MV) WD1247+042 See also (PE) WD1247+381 See also (QJ) WD1247+550 Possibly the coolest known degenerate star, Ref.(5S)See Also(5N)(MQ)(NN)(OK). WD1247-176 Name for MS companion EC 12477-1738B, PCEB(QH) WD1248+009 See also (NC) WD1248+161 See also (PD)(MV) WD1248-610 (P.Bergeron Finding Chart) WD1249+016 See also (QJ)(NC) WD1249+044 ZZ Ceti (OC) WD1249+160 See also (OK) WD1249+182 See also (PP) WD1249+450 See also (NC) WD1250-018 See also (QJ)(NC) WD1250-226 The central star of the Planetary Nebula A3, is a binary consisting of a white dwarf and a cool G8 IV star.(HD) WD1251+561 Reclassified as M star + nearby bright star; Ref.(QB) WD1251+584 See also (NC) WD1252+031 See also (NC) WD1252+559 MS+MS superposition; Ref. QB)See also (NC) WD1252+564 See also (PD)(MV) WD1253+024 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD1253+261 Central Star of PN LoTr 5, Ref.(JV) See also (SM) WD1253+378 HZ 34 is classified DAO in Ref.(DN)(JE)N. WD1253+385 Reclassified as M star; Ref.(QB) WD1254+003 ZZ Ceti candidate (HC) WD1254+019 See also (QJ)(NC) WD1254+223 See also (PP)(PM)(JV)(NL)(RK)(SM) WD1254+345 HS1254+3430 is a magnetic degenerate, Ref.(63). WD1254+428 See also (NC) WD1255+431 See also (RS) WD1255+481 See also (NC) WD1255+552 See also (NC) WD1255-019 See also (OY) WD1257+037 See also (OJ)(NN) WD1257+047 Finding chart for GD 267B Ref.(LJ) See also (PP) WD1257+278 See also (QA)(MY)(RT)(RY) WD1257-723 (P.Bergeron Finding Chart) WD1258+013 ZZ Ceti star Ref.(KA) NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog. See also (OK) WD1258+593 Finding chart for GD 322B Ref.(LJ) WD1259+053 See also (QJ)(NC) WD1300+062 Reclassified as M star; Ref.(QB) WD1300+263 See also (NN) WD1300-005 See also (OK) WD1302+412 See also (OY) WD1302+597 GD323 is classified DAB (peculiar). First known stratified H/HE atmosphere? Ref.(5W)(4K). See also (QM) WD1304+227 Common proper motion pair. See also (NZ)(PR) WD1305+125 See also (NC) WD1305+627 See also (OY) WD1305-017 See also (OK) WD1307+354 GD 154 is a ZZ CETI variable, Ref.(8Y) See also (PB)(PA)(NL) WD1307-017 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD1307-141 Name(s) for MS companion(s). EC 13077-1411B WD1308+537 See also (NC) WD1309+853 A new magnetic degenerate with a 4.9 Mg field (8N) See also (MV)(OJ) WD1310+583 See also (OJ) WD1310+597 See also (NC) WD1310-230 An interacting double-degenerate binary star with a period of 65.1 min. (FL) See also (SM) WD1310-472 A new, very low luminosity, degenerate star, one of the intrinsically faintest white dwarfs known, Ref.(9E) See also (OJ). WD1311+028 See also (QJ)(NC) WD1312+098 PG1312+098 is a magnetic degenerate, Ref.(9Z). WD1312+156 See also (NC) WD1314+003 See also (MS)(NR) WD1314+293 HZ43 soft X-ray EUV source, Ref.(7C) See also (QP)(QM)(JV)(NL)(OK)(PR)(RK)(SM) WD1314-153 The star indicated in both the Marsh and Arizona finding charts is at 13 16 47.5 -15 36 05 This is not consistent with the coords above which are for LP737-047, LHS2712 and NLTT33503. Also the coordinates on the Marsh chart are not consiste WD1315-110 See also (QV)(QA) WD1315-781 See also (OJ) WD1317+018 See also (QJ)(NC) WD1317+117 See also (NC) WD1317+135 See also (PD)(MV) WD1317+453 Newly identified double degenerate close binary, Ref.(7G)(JV). See also (QX) WD1318+042 See also (NC) WD1318+664 See also (NC) WD1319+019 See also (QJ) WD1320+645 See also (OK) WD1320-026 See also (NC) WD1321+083 See also (QJ) WD1321+305 See also (PE) WD1321+545.1 See also (NC) WD1322+130 See also (NC) WD1323+656 See also (RS) WD1323-514 (P.Bergeron Finding Chart) WD1324+004 See also (QJ)(NC) WD1324+458 WD/MS eclipsing binary system. Ref.(PH) See also (QX)(QH) WD1324+458.1 See also (PH) WD1325+581 See also (JV) WD1326+120 See also (QJ)(NC) WD1326+127 WD+MS Eclipsing Binary System. Ref.(QN). WD1326+132 See also (QJ)(NC) WD1327+594 See also (MV) WD1327-083 1400a absorption feature, Ref.(CL). See also (KP)(NB)(NL)(OJ) WD1328+017 See also (NC) WD1328+089 See also (QJ) WD1328+307 G165-007 has more identifiable line features than any other known degenerate, Ref.(DA)(QA). WD1328+461 See also (NC) WD1328+648 Spectrum shows Na I, Ref.(JJ) WD1329+666 See also (NC) WD1330+015 G62-46 is an unresolved double degenerate with a magnetic DA and a DC white dwarf, Ref.(24) See also (PS)(MV) WD1330+643 See also (OY) WD1331+111 See also (NC) WD1332+643 See also (PD)(MV) WD1333+005 MS companion=LP618-014B Eclipsing Binary System. Ref.(QN) See also (QP) WD1333+130 See also (QJ) WD1333+152 See also (QJ) WD1333+487 Spectroscopic composite DB + DM, Ref.(1V),Triple-star system: DB3.2+dM4+dM6.5 Ref.(QO). See also (QP) WD1333+510 See also (JV) WD1333-012 See also (NC) WD1334+013 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD1334+039 See also (OJ)(NN) WD1334+070 Single-lined double-degenerate binary. Ref.(PP) WD1334-001 See also (OW) WD1334-001.1 See also (NC) WD1334-160 See also (PP)(MY)(PQ)(PR) WD1334-326 PCEB. Ref.(QH) MS companion=EC 13349-3237B WD1334-678 (P.Bergeron Finding Chart) WD1335+001 ZZ Ceti candidate (HC) WD1335-001 See also (PY) WD1336+123 Common proper motion pair. See also (PR) WD1336+422 See also (NC) WD1337+021 See also (QJ)(NC) WD1337+598 See also (NC) WD1337+705 See also (QA)(NL)(OK) WD1339+050 See also (QJ)(NC) WD1339+346 See also (PS) WD1339+606 Name(s) for MS companion(s). SBS 1339+606B See also (QP) WD1339+616 See also (NC) WD1339+659 See also (PD)(MV) WD1339-340 VR = 212 km/sec corrected for gravitational redshift ref.(MI) WD1341+036 See also (PM) WD1341+056 See also (QJ) WD1342+414 See also (NC) WD1342+443 Single WD model atmosphere does not fit balmer lines, Ref.(81) See also (OK). WD1342+672 See also (MS)(NR) WD1343-006 ZZ Ceti star Ref.(KB) WD1344+090 See also (QJ) WD1344+106 See also (QA)(OJ)(NN)(OH) WD1344+572 See also (QP) WD1345+238 Common proper motion binary Ref.(JP) See also (PF)(OJ)(NN)(PR) WD1345+417 See also (NC) WD1346+188 WD+MS Eclipsing Binary System. Ref.(QN) See also (QH) WD1347+029 See also (RS) WD1347+477 See also (NC) WD1347-129 Eclipsing binary (EH) See also (PP)(SM) WD1348+400 DA; binary nature questionable. (Ref.(QB)See also (NC) WD1348+442 See also (OK) WD1348-273 See also (PR) WD1349+144 Double-lined double-degenerate binary. Ref.(PP)See also (JE) WD1349+545 SBS1349+5434 is a magnetic degenerate, Ref.(5T). See also (PD) WD1349+552 ZZ Ceti star ref.(KA)(OC) See also (PB)(OK) WD1349-230 See also (OR) WD1350+457 See also (NC) WD1350+656 ZZ CETI variable, Ref.(87)(JE)N. See also (PB)(NQ)(OK) WD1350-090 WD1350-090 is a magnetic degenerate, Ref.(9W) See also (OJ). WD1351+489 A new pulsating DB star, Ref.(DV). WD1352+004 See also (OR) WD1352+013 ZZ Ceti star Ref.(KB) WD1352+421 Irradiated secondary star. Ref.(QB) WD1352-022 See also (NC) WD1353+409 See also (RL) WD1354+340 CPMB WITH BD+34 2473 See also (NZ)(PQ) WD1357+366 See also (NC) WD1359+256 See also (QJ) WD1400+005 See also (OK) WD1401+005 Conflicting locations - Aladin image is centered on Marsh's ID while Arizona ID is the blue star directly to the right of center. WD1401+051 See also (MS) WD1401+438 See also (SM) WD1401-014 See also (NC) WD1401-147 ZZ Ceti star ref.(KA) WD1402+545 See also (NC) WD1403+043 See also (NC) WD1403+451 See also (NC) WD1403-077 See also (PP)(JV) WD1404+008 See also (NC) WD1404+603 See also (QJ)(NC) WD1405+008 See also (OY) WD1406+050 NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog, WD1407+425 See also (QA)(OK) WD1407-023 See also (RF)(RS) WD1407-475 Variability in radial velocity indicates a possible binary with a period of ~ 1 day. (EE) (P.Bergeron Finding Chart) WD1408+323 See also (QP)(QC) WD1408-018 WD+MS Eclipsing Binary System. Ref.(QN) See also (NC) WD1409+107 PCEB. Ref.(QH). WD1409+233 WD+MS Eclipsing Binary System. Ref.(QN). WD1410+051 See also (OY) WD1410+168 See also (PP) WD1410+269 See also (QJ) WD1411+659 See also (PE)(NC) WD1412+612 New magnetic degenerate, Ref.(63). WD1412-013 PCEB. Ref.(QH) See also (QJ)(NC) WD1412-049 Name(s) for MS companion(s). PG 1412-049B WD1413+015 WD/MS eclipsing binary system. Ref.(PH) See also (QH)(NL)(QN) WD1413+241 See also (RY) WD1414+012 ZZ Ceti star Ref.(KB) WD1414+020 See also (QJ)(NC) WD1414+350 See also (PE) WD1414-088 Component B of the double-lined DA+DA binary system HE 1414-0848. (HG) WD1414-088.1 Component A of the double-lined DA+DA binary system HE 1414-0848. (HG) WD1415+132 See also (QJ) WD1416+060 binary nature questionable.Ref.(QB) WD1416+077 See also (QJ) WD1416+259 Possible unresolved DA/DC spectroscopic binary. Ref.(PD) WD1416+633 Binary (WD+dM) system. Ref.(MK) WD1416+644 See also (PR) WD1417+473 See also (QJ)(NC) WD1418-088 Double degenerate system. Ref.(JP) WD1419+252 Has an Unresolved companion DA5.0 White Dwarf with (Vmag = 18.10 AbsMag = 12.14) Ref(QC) WD1419+576 Resolved triple (WD+dM2+dM2) system. Ref.(MQ) See also (QP) WD1420+441 Possible double-degenerate system. Ref.(QS). WD1420+518 See also (NC) WD1421+243 WD/MS eclipsing binary system. Ref.(PH) See also (QN) WD1421+527 See also (RS) WD1422+095 CX BOO is a ZZ CETI variable, Ref.(44). See also (PP)(PB)(SF) WD1422+497 See also (NC) WD1423+027 See also (QJ)(NC) WD1423+371 See also (NC) WD1424+534 PG1159 DO degenerate, Ref.(DN); type A, Ref.(66). WD1424+602 See also (NC) WD1425+375 See also (PD)(MV) WD1425+540 G200-39 common proper motion binary with G200-40 (K dwarf). Prototype of the class of DBA stars, Ref.(5R). WD1425-811 L0019-002 is a ZZ CETI variable, Ref.(7I) See also (PP)(PB)(8Z)(NB)(NL)(OD) WD1426-276 See also (PP) WD1427-024 See also (QJ)(NC) WD1428+114 See also (QJ) WD1428+373 Double-degenerate system. Ref.(QX) See also (PS)(OK) WD1428+582 PCEB. Ref.(QH). WD1429-037 ZZ Ceti (OC) WD1429-121 Non-radial g-mode pulsator Ref.(KO) WD1430+041 See also (RS) WD1430+070 See also (QJ) WD1430+432 See also (PD)(MV) WD1430+460 See also (PD)(MV) WD1431+614 See also (NC) WD1432-164 PCEB. Ref.(QH). WD1433+367 See also (QJ)(NC) WD1433+377 WD/MS eclipsing binary system. Ref.(PH) See also (QJ)(NC)(QH) WD1433+538 See section A5.15 in Ref. (LJ)MS companion=GD 337B See also (QJ)(QH)(PE)(NC) WD1434+289 See also (PS) WD1434+503 Double-degenerate merger system. Ref.(QT)(SL). WD1435+370 Name(s) for MS companion(s). CBS194B WD1435+383 See also (QJ)(NC) WD1435+433 DA; binary nature questionable.Ref.(QB) WD1435+621 See also (NC) WD1436+424 See also (NC) WD1436+526 See also (OK) WD1436+578 See also (NC) WD1436-216 Name(s) for MS companion(s). EC 14363-2137B WD1437+102 Possible double-degenerate system. Ref.(QS). WD1437+368 See also (NC) WD1437+417 See also (QJ) WD1437-008 See also (QJ)(NC) WD1440+003 See also (QJ)(NC) WD1440+017 ZZ Ceti star Ref.(KB) WD1440+753 See also (OQ)(MV)(NO)(RK) WD1441-007 See also (OK) WD1443+336 Name(s) for MS companion(s). PG 1443+336B See also (QP) WD1443+414 DA; binary nature questionable.Ref.(QB) WD1443+590 See also (RS) WD1444+102 See also (QJ) WD1444+592 See also (PD)(MV) WD1444+636 See also (QM) WD1444+636 See also (JV) WD1444-174 See also (OJ)(NN) WD1445+414 See also (NC) WD1446+050 DA; binary nature questionable.Ref.(QB)See also (NC) WD1446+575 See also (MS)(NR) WD1447+356 See also (QJ)(NC) WD1447-190 Reported as sdB in an earlier Ref. (EH). WD1448+077 See also (PP) WD1448+419 See also (QJ)(NC) WD1449+003 G066-036 common proper motion binary with G66-35 (G5 dwarf), Ref.(75). SectionA2.2 in Ref.(LJ) reports different motions for the pair therfore not CPMB. See also (PQ) WD1449+168 Finding chart for PG 1449+168B Ref.(LJ) See also (PP) WD1449+522 DA binary nature questionable.(faint star nearby); Ref.(QB)See also (NC) WD1449+559 See also (QJ)(NC) WD1450+011 See also (QJ)(PE)(NC) WD1451+006 NOTE: Simbad currently shows coordinates for WD1451+006.1 not WD1451+006 See also (PP)(MZ) WD1451+006.1 Mistakenly identified as WD1451+006 in Ref. (MH) See also (OK) WD1451+411 See also (QJ)(NC) WD1452+435 See also (PD)(MV) WD1452+553 See also (OK) WD1452-022 See also (NC) WD1454+163 WD+MS Eclipsing Binary System. Ref.(QN). WD1454+486 See also (NC) WD1454+595 See also (QJ)(NC) WD1454+614 See also (NC) WD1454-630.1 L151-81 a rare binary with DA and DB components, Ref.(8A). WD1454-630.2 L151-81 a rare binary with DA and DB components, Ref.(8A). WD1455+298 Possible binary (OH) See also (QA)(PS)(OR) WD1456+103 CW BOO is a non-radial pulsator, Ref.(44). WD1456+106 See also (QJ) WD1456+475 See also (RS) WD1456+515 DA; binary nature questionable.Ref.(QB) See also (NC) WD1457+349 See also (QJ)(NC) WD1457+455 DA; binary nature questionable.Ref.(QB) See also (NC) WD1457+462 DA; binary nature questionable.Ref.(QB) See also (NC) WD1457-086 See also (QV)(QD)(QA)(PP) WD1458+045 See also (NC) WD1458+171 Name(s) for MS companion(s). PG 1458+171B See also (QP) WD1459+001 ZZ Ceti star Ref.(KB) NOTE: Ref(LM) uses WD numbers based on 2000 coordinates which do not agree with WD numbers in this catalog. WD1459+013 See also (PJ)(NC) WD1459+333 See also (OK) WD1459+347 See also (MY)(OK) WD1500+011 See also (NC) WD1500+447 See also (NC) WD1500-170 See also (PP) WD1501+664 H1504 may be the hottest known star,H and He lines absent;high gravity OVI features; HEAO-1 A-2 and EXOSAT powerful soft X-ray source, Ref.(7X); type EP, Ref.(66)(JV)(KL). WD1502+324 See also (QJ)(NC) WD1502+349 Name(s) for MS companion(s). CBS223B WD1502+586 See also (NC) WD1503+331 DA + some red excess; Ref.(QB)See also (NC) WD1503-070 See also (MV) WD1503-093 See also (PP) WD1504+006 See also (QJ)(NC) WD1504+546 Name(s) for MS companion(s). CBS301B See also (QP) WD1504-011 PCEB. Ref.(QH) See also (QJ)(NC) WD1504-770 (P.Bergeron Finding Chart) WD1505+483 See also (NC) WD1506+399 See also (PD)(MV) WD1506-019 DA; binary nature questionable.Ref.(QB) WD1507+021 See also (PP) WD1507+434.1 See also (NC) WD1507-105 See also (PP) WD1508+008 See also (QJ)(NC) WD1508+025 See also (QJ)(NC) WD1508+409 See also (QJ)(NC) WD1509+020 See also (QJ)(NC) WD1509+322 See also (NB) WD1509+425.1 See also (MV) WD1510+566 See also (OK)(PR) WD1511+009 See also (PP)(OK) WD1511-048 Single-lined double-degenerate binary. Ref.(PP) WD1514+353 See also (NC) WD1514+411 See also (PR) WD1516+348 DA; binary nature questionable.Ref.(QB) WD1516+460 See also (QJ)(NC) WD1516+534 See also (NC) WD1516+612 See also (PD)(MV) WD1517+502 A rare dwarf carbon star plus white dwarf binary, Ref.(5I),(MQ)Reclassified as carbon star; Ref.(QB) See also (NC) WD1517+740 HS1517+7403 is a PG1159 star with no detected variability, Ref.(DI); type A, Ref.(66). WD1518+328 See also (QJ)(NC) WD1518+381 DB; binary nature questionable.Ref.(QB)See also (NC) WD1519+323 See also (NC) WD1519+422 See also (QJ) WD1519+500 See also (OK) WD1519+611 See also (NC) WD1520+388 See also (NC) WD1520+525 PG1520+535 is a PG1159 star with a detected planetary nebula but no detected variability, Ref.(DI) DO degenerate, Ref.(DN). WD1521+310 See also (JE) WD1521+352 DA; binary nature questionable.Ref.(QB) WD1521-003 ZZ Ceti star Ref.(KB) WD1522+462 See also (QJ)(NC) WD1522+479 See also (NC) WD1522+508 Name for MS companion CBS318B See also (QP)(QH) WD1522+662 See also (JV) WD1524+005.1 See also (NC) WD1524-749 (P.Bergeron Finding Chart) See also (PP) WD1526+005 PCEB Ref(QH) See also (QJ)(NC) WD1526+013 See also (OK) WD1526+333 See also (NC) WD1526+348 See also (QJ)(NC) WD1528+087 Post-common envelope binary. Ref.(QB) WD1528+487 See also (QM) WD1529+141 See also (OJ) WD1529-772 See also (MV)(RK) WD1530+037 See also (NC) WD1530+315 Reclassified as M star + nearby bright star; Ref.(QB) WD1530-019 NOTE: 2000 coords are from ref(MH),Ref(LU) gives J153332.9-020600.0 but no star found at these coords using SDSS Finding Chart Tool. WD1531+746 ZZ Ceti (OC) WD1531-022 See also (MY) WD1532+033 See also (NL) WD1532+394 See also (QJ)(NC) WD1532+415 See also (QJ)(NC) WD1532+420 See also (NC) WD1533+423 See also (PD)(MV) WD1533-057 New magnetic degenerate, Ref.(5U)(JE)N. WD1534+503 Double degenerate system? Radial velocities -106/159? Ref.(JP) See also (OK) WD1537+382 See also (NC) WD1537+532 See also (PD)(MV) WD1537+651 See also (JE) WD1537-006 DA; binary nature questionable.(Ref. QB)See also (NC) WD1537-152 See also (PP) WD1538+333 See also (OJ) WD1539+035 See also (QJ)(NC) WD1539+039 See also (PD)(MV) WD1539+333 See also (NC) WD1539+530 Finding chart for PG 1539+530B see A5.11 in Ref.(LJ) WD1541+061 See also (NC) WD1541+297 DA; binary nature questionable.(Ref. QB) WD1541+558 See also (NC) WD1541+650 ZZ Ceti star ref.(JE)(OC) WD1541-381 See also (PP)(SM) WD1542+182 See also (QD) WD1542+392 Reclassified as M star; Ref.(QB) WD1542-275 Common proper motion pair. See also (PR) WD1543+332 See also (NC) WD1544+009 CPMB system with the G0 star BD+01 3129. Ref.(OF)(PR) WD1544+218 See also (QJ) WD1544-377 L481-60 common proper motion binary with HR5965 (G6 dwarf) See also (PP)(OS)(MV)(NL)(OJ)(PR) WD1545+303 See also (NC) WD1545+495 See also (NC) WD1546+316 See also (NC) WD1546+376 See also (QJ)(NC) WD1546+426 See also (MS) WD1547+015 See also (PP) WD1547+390 See also (QJ)(NC) WD1547+411 WD/MS eclipsing binary system. Ref.(PH) See also (QJ)(NC)(QH)(QN) WD1548+405 See also (OK) WD1548+539 See also (QJ)(NC) WD1549-000 Correct Declination is +00 04 16 (1950). (DY) WD1550+130 WD/MS eclipsing binary system. Ref.(PH)(QH) WD1550+183 See also (PP) WD1550+437 See also (NC) WD1551+051 See also (NC) WD1552+248 See also (QJ) WD1552+486 See also (MS) WD1553+414 See also (QJ)(NC) WD1554+322 See also (OK) WD1554+550 See also (NC) WD1555+366 See also (NC) WD1555+401 See also (NC) WD1555-089 See also (PQ) WD1556+026 See also (NC) WD1556+085 See also (QJ) WD1556+268 PCEB. Ref.(QH). WD1558+378 Reclassified as M star; Ref.(QB)See also (NC) WD1558+616 Name(s) for MS companion(s). HS 1558+6140B WD1559+343 See also (NC) WD1559+365 Irradiated secondary star; Cataclysmic variable? Ref.(QB)See also (QJ)(NC) WD1559+366 See also (NC) WD1559+369 R808 is a ZZ CETI variable, Ref.(7M) See also (PB)(NL) Polarized magnetic WD. Ref.(RG). WD1559+534 See also (OK) WD1600+308 See also (OK) WD1600+472 DA; binary nature questionable.Ref.(QB)See also (NC) WD1601+581 See also (QP) WD1602+543 See also (NC) WD1603+432 See also (QP) WD1603+492 See also (PD)(MV) WD1604+463 See also (QJ)(NC) WD1605+089 See also (QJ) WD1605+424 See also (QJ)(NC) WD1605+428 See also (QJ)(NC) WD1606+422 Double degenerate system. Ref.(JP) See also (NB) WD1608+002 See also (QJ)(NC) WD1608+258 See also (NC) WD1609+011 See also (QJ)(NC) WD1609+044 See also (PP) WD1609+135 See also (PP)(OJ)(MY) WD1609+468 See also (QJ)(NC) WD1609+493 See also (QJ)(NC) WD1611+459 See also (NC) WD1611-084 See also (QM) WD1613+458 See also (OW) WD1614+136 See also (RL) WD1614+160 See also (QV) WD1615+390 See also (NC) WD1615-154 See also (PP)(NB)(NL)(OK) WD1616+010 See also (QJ)(NC) WD1616+430 See also (NC) WD1616+435 ZZ Ceti star Ref.(KB) WD1617+064 Wide-binary? Ref.(QB) WD1618-507.1 (P.Bergeron Finding Chart) WD1619+123 Companion to HD 147528 Ref.(LJ) WD1619+414 Name(s) for MS companion(s). KUV 16195+4125B WD1619+525 Tertiary companion may be dM2; physical association of the three stars uncertain. Ref.(QO). See also (QR)(QP) WD1620-391 CD-38 10980 25,000k DA degenerate with gravitational redshift, Ref.(CB)(JV), Companion to HD 147513.(LJ) See also (PP)(OS)(MV)(NL)(OK)(OJ)(PR) WD1621+347 See also (QJ)(NC) WD1621+360 See also (NC) WD1621-002 See also (QJ)(NC) WD1621-010 See also (NC) WD1622+141 Reclassified as M star + nearby bright star; Ref.(QB) WD1622+323 Name(s) for MS companion(s). PG 1622+323B See also (QP) WD1622+369 See also (QJ)(NC) WD1622+406 See also (NC) WD1623+366 Probable double-degenerate system. Ref.(QT). WD1623-540 See also (PR) (P.Bergeron Finding Chart) WD1624+235 See also (QJ) WD1625+125 ZZ Ceti (OC) WD1626+291 See also (NC) WD1626+368 See also (PS)(OJ)(NB) WD1627+129 See also (QJ) WD1626+495 See also (RF)(RS) WD1628+390 See also (OK) WD1628-873 (P.Bergeron Finding Chart) WD1631+781 DA + DM detached binary RE1629+780, Ref.(AJ)(JV). Resolved triple (WD+dM3+dM3) system. Ref.(MQ) See also (QP)(QO)(QM)(NL)(RK)(SM)(SM) WD1632+177 See also (QA)(OJ) WD1632+387 DA; binary nature questionable.Ref.(QB)See also (NC) WD1633+313 See also (NC) WD1633+433 Member of binary or multiple star system. Ref.(OJ) See also (OH) WD1633+572 CPM companion of CM Dra, Ref.(JV) See also (OJ)(PR) WD1634-573 Hot (55,000K) DO degenerate with photospheric carbon in UV; hottest white dwarf with Einstein redshift, Ref.(AH)(AS)(JV). WD1635+252 See also (NC) WD1635+315 See also (NC) WD1635+478 See also (NC) WD1636+057 See also (PP) WD1636+351 See also (QP)(JV)(NL) WD1637+335 See also (NB) WD1639+153 See also (MY) WD1639+211 See also (NC) WD1639+537 Only single magnetic degenerate with emission lines, Ref.(2H) See also (MV) WD1640+113 See also (PP) WD1640+384 See also (NC) WD1641+114 See also (PP) WD1641+241 See also (PD)(MV) WD1641+387 See also (JV) WD1643+143 Name(s) for MS companion(s). PG 1643+143B See also (QP) WD1643+425 See also (NC) WD1644+234 See also (QJ) WD1644+424 PCEB (QH) See also (QJ)(NC) WD1645+251 See also (NC) WD1645+325 The first known pulsating DB white dwarf, Ref.(DW) See also (QP)(NB) WD1645+372 See also (PD)(MV) WD1646+062 Name(s) for MS companion(s). PG 1646+062B WD1646+282 PCEB. Ref.(QH). WD1646+361 See also (NC) WD1647+591 G226-029 is a ZZ CETI variable, Ref.(7J); 1400A absorption, Ref.(3N) See also (PB)(PO)(MY)(NB)(NL)(OE)(OJ) WD1648+342 See also (PD)(MV) WD1648+371 See also (RY) WD1648+391 See also (QJ)(NC) WD1648+407 See also (JV)(NO) WD1649+300 See also (NC) WD1649+419 See also (NC) WD1650+355 See also (PD)(MV) WD1653+188 See also (NC) WD1653+200 See also (NC) WD1653+256 ZZ Ceti Candidate (Ref. JL) WD1653+385 See also (PV)(OJ) WD1654+160 V824 HER is a non-radial pulsator, Ref.(44), see section A5.23 in Ref.(LJ). WD1655+215 See also (PP)(OJ)(NB) WD1656-062 See also (PR) WD1657+321 See also (OJ) WD1657+343 See also (RK)(OK)(JV) WD1658+440 Ultra-massive DA degenerate 1.31 MSUN, low B-field, X-ray source, Ref.(9U) See also (QP)(OQ)(8L)(5V)(JV)(MV)(RL)(RK) WD1659+303 Finding chart for PG 1659+303B see A5.24 in Ref.(LJ) WD1659+344 See also (NC) WD1659+359 ZZ Ceti star Ref.(KB) WD1659+442 See also (JV) WD1659-531 BPM24601 common proper motion binary with HR6314 (F7 dwarf). Additional updated chart by P.Bergeron 3/20/07 - Click T.R.Marsh Chart. See also (NB)(PR) WD1701+596 See also (RF)(RS) WD1702+322 See also (PD)(MV) WD1703+199 See also (QJ)(NC) WD1703+212 PCEB. Ref.(QH) See also (QJ)(NC) WD1703+261 See also (PR) WD1703+338 DA; binary nature questionable.Ref.(QB) WD1703+388 See also (QJ)(NC) WD1704+217 See also (NC) WD1704+481.1 Sanduleak-Pesch binary pair of DA stars,12,500K, 9500K masses 0.08 and 0.43 solar masses,first known triple degenerate,average radial velocity=0.6km/sec, Ref.(9Q)(2E)(FH). WD1704+481.2 Sanduleak-Pesch binary pair of DA stars,12,500K, 9500K masses 0.08 and 0.43 solar masses,first known triple degenerate,average radial velocity=0.6km/sec, Ref.(9Q)(2E)(FH). WD1705+030 See also (PV)(OJ) WD1706+220 See also (NC) WD1706+332 See also (PQ) WD1707+295 See also (NC) WD1707+427 PG1159 DO degenerate, Ref.(DN); type A, Ref.(66) variable WD Ref(KL) Non-radial g-mode pulsator Ref.(KO)N. WD1708+437 See also (QX) WD1709+230 See also (OR) WD1709-575 (P.Bergeron Finding Chart) WD1710+559 See also (NC) WD1710+683 Binary (DA7.2+K7/M0 dwarf) system. Ref.(MK) See also (PQ)(PR) WD1711+305 MS+MS superposition; Ref.(QB) WD1711+657 ZZ Ceti star Ref.(KB) WD1711+668 See also (QM) WD1712+274 See also (NC) WD1712+298 See also (NC) WD1712+629 See also (QJ)(NC) WD1713+332 Double degenerate close binary, Ref.(7G). WD1713+393 See also (MV) WD1713+695 See also (QP) WD1714-547 ZZ Ceti star ref.(KA) (P.Bergeron Finding Chart) WD1715+547 See also (NC) WD1715+601 See also (PD)(MV) WD1716+020 Common proper motion binary. Ref.(JP) See also (PP)(NB)(PR) WD1716+598 See also (NC) WD1717+610 PCEB. Ref.(QH) See also (QJ)(NC) WD1717-345 Possible red dwarf companion, Ref.(8P) See also (QO) WD1719+560 See also (QJ) WD1719+562 See also (PD) WD1719+569 See also (QJ)(NC) WD1719+629 See also (NC) WD1720+283 See also (NC) WD1720+638 See also (NC) WD1722+541 See also (PD)(MV) WD1723+553 Post-common envelope binary; irradiated secondary star. Ref.(QB) WD1723+563 PCEB Ref.(QH) See also (QJ)(QH)(NC) WD1723+586 ZZ Ceti star Ref.(KB) See also (NQ)(NL) WD1723+595 See also (NC) WD1724+626 See also (QJ)(NC) WD1724-359 See also (RK) WD1725+561 See also (QJ)(NC) WD1725+586 See also (QM)(NO)(OK)(RK) WD1726+545 Post-common envelope binary. Ref.(QB)See also (QJ)(NC) WD1726-578 (P.Bergeron Finding Chart) WD1727+589 See also (NC) WD1728+565 See also (PD)(MV) WD1728+621 See also (QJ)(NC) WD1729+371 Contains circumstellar dust (NG) See also (QD)(QA)(OJ)(MR) WD1730+625 PCEB. Ref.(QH) See also (QJ)(NC) WD1731+591 ZZ Ceti star Ref.(KB) WD1732+608 See also (NC) WD1733-544 (P.Bergeron Finding Chart) WD1734+542 See also (NC) WD1734+742 Cataclysmic Variable of the RS CVn-type. Ref.(SM) WD1735-318 An extremely hot DA white dwarf close to the open cluster NGC6405, Ref.(4P). WD1736+052 See also (PP) WD1736+133 White dwarf companion to HD160365, Ref.(36). WD1736+540 See also (NC) WD1736+562 See also (NC) WD1738+669 Hottest known DA star associated with nebula, Ref.(12). WD1740+541 See also (NC) WD1740-706 See also (QM)(RL) WD1741+543 See also (NC) WD1743-521 (P.Bergeron Finding Chart) WD1748+708 G240-072 is magnetic and polarized, Ref.(03) See also (MV)(NB)(NN)(OJ) WD1750+098 EG124 common proper motion binary with G140-b1a / BD+09 3501 (K2 dwarf) See also (PQ). WD1751+106 ABELL 43 is a hybrid, PG1159-like central star; type LGEH, Ref.(66) CSPN effective temperature 116,900K. (IO)N. WD1756+143 See also (OJ) WD1756+827 See also (OJ)(MM)(NB)(NN)(OL) WD1800+685 See also (QP)(NL)(RK) WD1802+213 See also (JV) WD1803-482 RS CVn variable. Ref.(SM) WD1814+248 A new magnetic degenerate, Ref.(8M). WD1815+381 Variable polarized magnetic WD. Ref.(RG). WD1818+126 See also (MV) WD1819+580 See also (QM)(RK) WD1820+609 See also (OJ) WD1821+643 PG1159 DO degenerate, type LGE, Ref.(66)(JV)(KL) Non-radial g-mode pulsator Ref.(KO) See also (RN) WD1822+008 SH2-68 is a PG1159-type planetary nucleus, type AH, Ref.(66) CSPN effective temperature 125,900K. (IO)N. WD1822+410 See also (QA)(OB) WD1823+063 NGC6633:LA15 = NGC6633:LAWDS15 Not DAZ, observed CaII probably interstellar, Private Communication Williams,K.A. 08/14/2009 WD1824+040 Double-degenerate candidate Ref.(KP), Triple degenerate system DA3.4(a)+DC5.0(b)+DC10.6(c) see A5.1 in Ref.(LJ) Finding chart for G21-15C See also (PP) WD1824+062 NGC6633:LA 8 = NGC6633:LAWDS 8 Not DAZ, observed CaII probably interstellar, Private Communication Williams,K.A. 08/14/2009 WD1824+063 Calculated Mv=11.84 from model spectrum and radius and conclude star is too bright to be a member of NGC6633. (ED) nOTE: NGC6633:LA14 = NGC6633:LAWDS14 WD1824+063.1 NGC6633:LA27 = NGC6633:LAWDS27 Not DAZ, observed CaII probably interstellar, Private Communication Williams,K.A. 08/14/2009 WD1824+063.2 NGC6633:LA13 = NGC6633:LAWDS13 WD1824+064 Possible double degenerate star, Ref.(MZ) Note NGC6633:LA 4 = NGC6633:LAWDS 4 WD1824+600 ZZ Ceti (OC) WD1825+063 Possible double degenerate star, Ref.(MZ) Note NGC6633:LA 7 = NGC6633:LAWDS 7 WD1825+067 NGC6633:LA16 = NGC6633:LAWDS16 WD1826+064 NGC6633:LA12 = NGC6633:LAWDS12 WD1826-045 See also (QV)(OH) WD1827-106 Temperatures ambigious. Ref.(PP) See also (OD) WD1829+547 G227-035 is a magnetic white dwarf, Ref.(03) See also (OJ). WD1830+721 HS1830-721 is an intermediate temperature DO star with TEFF > 80,000K, Ref.(2T). WD1831-002 White dwarf companion of a binary pulsar, Ref.(9S). WD1833+644 Possible triple-star system: DA2.0 with dM3+dM6.5 companions. Ref.(QO). See also (QP) WD1834-781 (P.Bergeron Finding Chart) See also (PP) WD1837-619 Strong UV lines of neutral carbon, Ref.(CI). WD1840+042 See also (MY) WD1844-223 See also (PP)(RK) WD1844-654 See also (JV) WD1845+019 Single-lined double-degenerate binary. Ref.(PP)See also (NL)(RK) WD1845+683 White dwarf is likely, neither a suspected nor confirmed binary. Ref. (MQ) See also (PS)(NL)(NO)(RK) WD1855+096 White dwarf companion of a binary pulsar, Ref.(9S). WD1855+338 G207-009 is a ZZ CETI variable, Ref.(8Z) See also (PB)(MY)(NL) WD1856+534 A possible triple system, Ref.(7Z). WD1857+119 See also (PP) WD1858+393 See also (QA)(MR)(OH) WD1900+140 Central star of SH2-28; type A, Ref.(66). WD1900+705 G260-015 is a magnetic white dwarf, Ref.(06)(03). See also (NB)(OJ) WD1906-600 See also (JV) WD1909+304 PG1159-like central star of NGC6765; type lgE, Ref.(66). WD1910+047 Photospheric X-ray emission detected by HEAO-B, TEFF= 22,500K, Ref.(7D)(7B)(JV). WD1911+135 See also (PP)(PQ) WD1914+094 See also (PP) WD1917+386 See also (OJ) WD1917-077 LDS678A shows strong CI lines in UV, weak HeI in optical, Ref.(CF)(AO), Binary DA+dm3.5, Ref.(LJ) See also (PV)(OJ)(PR). WD1918+376 See also (OS) WD1919+145 See also (OJ)(NB)(NL) WD1919+37602 Possible non-cluster WD. Ref.(NX) WD1919+37603 Possible non-cluster WD. Ref.(NX) WD1919+37605 Possible non-cluster WD; possible DA+dM binary system. Ref.(NX) WD1919+37608 See also (OS) WD1919+37610 Possible DA+dM binary system. Ref.(NX) WD1921-566 See also (RK) WD1929+011 See also (QV) WD1930+278 See also (QX) WD1932-136 See also (PP)(PR) WD1935+276 G185-032 is a ZZ CETI variable, Ref.(7J) See also (PB)(NL)(OD)(OJ) WD1936+327 See also (MZ)(NL) WD1940+374 See also (OE) WD1942+499 See also (NB)(NO)(RK) WD1943+163 See also (PP) WD1944-421 See also (JV)(SM) WD1950+250 GR394 is a ZZ CETI variable, Ref.(86). See also (PB) WD1950-432 See also (PP)(NO) WD1953-011 See also (PP)(OJ)(MM)(NB)(NL)(OL) WD1953-715 (P.Bergeron Finding Chart) WD1957+225 Central star of PN. Ref.(QM) See also (QP) WD1958+015 K1-18 is a PG1159-like central star of NGC6852, type lgE, Ref.(66). WD1959+059 See also (PP) WD2002-110 See also (OJ)(NN) WD2003+437 GD387 probable unresolved DA+DC system, Ref.(23). WD2003+542.1 See also (QX) WD2004-605 See also (QM)(PP)(RK) WD2007-219 See also (PP) WD2007-303 See also (QP)(PP)(OJ)(NB) WD2009+622 Name(s) for MS companion(s). GD 543B See also (QP) WD2010+310 GD229 is magnetic and polarized, Ref.(6)(03); UV spectrum discussed in Ref.(1Q). WD2011+398 PCEB DAQZ + dM3 binary. Ref.(RV)(10) See also(JV)(QO)(QM)(QH)(RK) WD2014-575 See also (JV)(NB)(NL)(NO) WD2019+756 MS+MS superposition; Ref.(QB) WD2020-425 Double-lined double-degenerate binary. Ref.(PP)See also (JV)(NO)(RK) WD2027+068 A new hot DO star with ultra highly excited ionization stages, Ref.(64). WD2028+390 See also (JV) WD2029+183 The finding charts point to different stars. WD2031-277 See also (JV) WD2032+188 Single-lined double-degenerate binary. Ref.(PP) See also (QX) WD2032+248 See also (PV)(OJ)(JV)(NB)(NL)(OE)(RX) WD2038-013 See also (NC) WD2039-001 See also (MS) WD2039-003 Reclassified as M star; Ref.(QB)See also (NC) WD2039-202 See also (PP)(OJ)(NL) WD2039-682 See also (PP)(OJ)(MV)(MY)(NB) WD2040-392 See also (OJ) WD2041-064 See also (NC) WD2043-053 See also (QJ)(NC) WD2043-073 See also (PD)(MV) WD2043-635 See also (NO) WD2044+001 See also (NC) WD2044-043 See also (PQ)(PR) WD2045+006 Low accretion rate polar. Ref.(QB) WD2045-000 See also (NC) WD2045-012 Reclassified as M star; Ref.(QB) WD2046+396 See also (NL) WD2046-059 See also (QJ)(NC) WD2047+372 See also (OJ)(NB)(NL) WD2047-000 Log g = 5; star is probably Main-sequence A-star. Ref.(QT). WD2048+263 Member of binary or multiple star system. Ref.(OJ) WD2048+809 See also (PQ)(PR) WD2048-002 See also (QJ)(NC) WD2048-250 See also (OJ) WD2049-004 See also (PD)(MV) WD2050-056 See also (RS) WD2051+464 See also (JV) WD2051-208 See also (PP) WD2052+006 MS+MS superposition; Ref.(QB)See also (NC) WD2053-011 DB; binary nature questionable.Ref.(QB) WD2054+005 See also (QJ)(NC) WD2054-050 See also (OJ)(NN) WD2055+221 See section A1.1 in Ref. (LJ). WD2056+033 See also (JV) WD2056-062 See also (QJ) WD2056-070 See also (NC) WD2058+342.1 GD 392B is ultracool CPMB companion to GD 392 Ref.(JP) WD2059+190 See also (MY) WD2059+316 Strong UV CI lines, Ref.(CK). WD2102+101 See also (NC) WD2103-061 See also (QJ)(NC) WD2104-070 See also (QJ)(NC) WD2105-820 See also (QV)(QA)(PP)(OJ)(MV)(NB)(NL) (P.Bergeron Finding Chart) WD2108+094 See also (QJ)(NC) WD2109+010 See also (QJ)(NC) WD2109+089 See also (RF)(RS) WD2109+100 See also (QJ)(NC) WD2110+102 DB; binary nature questionable.Ref.(QB) WD2110-006 MS+MS superposition; Ref.(QB) WD2111+498 See also (JV)(NB)(NL)(RX)(RK) WD2111-012 PCEB Ref.(QH) See also (QJ)(NC) WD2113+007 MS+MS superposition; Ref.(QB) WD2114+239 The DAO degenerate central star of ABELL 74, Ref.(66). WD2115+008 See also (QJ)(NC) WD2115+118 A new hot DAO star with ultra highly excited ionization stages, Ref.(64). WD2115+339 RXJ2117.1+3417 is a PG1159 star with 24 detected periods and an associated planetary nebula, Ref.(DF,BA); type lgE, Ref.(66)(JV) Non-radial g-mode pulstaor Ref.(KO)N. WD2115-082 See also (NC) WD2115-560 Contains circumstellar dust (NG) See also (QD)(QA)(PP)(OR)(OJ)(MV)(NB) WD2116+736 See also (QP)(NO)(RK) WD2116-005 Double-degenerate merger system. Ref.(QT). WD2117+539 1400A absorption feature, Ref.(CL) See also (PV)(NL)(OJ) WD2118-011 PCEB. Ref.(QH) See also (QJ)(NC) WD2118-061 See also (NC) WD2120+002 PCEB. Ref.(QH) See also (QJ)(NC) WD2120+054 See also (PP) WD2122+361 NGC7063:LA 3 = NGC7063:LAWDS 3 WD2122+362 NGC7063:LA 4 = NGC7063:LAWDS 4 WD2122+362.1 NGC7063:LA 1 = NGC7063:LAWDS 1 WD2122+362.2 NGC7063:LA 2 = NGC7063:LAWDS 2 WD2122+363 NGC7063:LA 6 = NGC7063:LAWDS 6 WD2122-013 WD is in a binary system with orbital period = 6.9 hours. Ref.(RU).See also (NC) WD2123-226 White dwarf companion to the barium star ZETA Cap with MWD=0.96Msun TEFF= 23,200K, Ref.(35). WD2124+191 PCEB. Ref.(QH)(RK) WD2124+550 See also (MY) WD2124-224 See also (QM)(PP)(RK) WD2126+734 1400A absorption feature, Ref.(2I), (3N), Binary system - companion probable WD, see section A5.7 in Ref.(LJ) See also (NL)(OJ) WD2126-069 Reclassified as M star + nearby bright star; Ref.(QB) WD2127+115 PG1159 star. Ref.(QB) WD2128+469 Eclipsing Binary system classified as a Cataclysmic Variable. (JF)(PH). See also (QH)(SM)(SM) WD2129+000 See also (PR) WD2129+003 PCEB. Ref.(QH) See also (QJ)(NC) WD2129-002 Reclassified as M star + nearby bright star; Ref.(QB) WD2130-047 See also (OB) WD2131+066 PG1159 DO degenerate, Ref.(DN); type A, Ref.(66) Binary system: PG1159+M2V (IJ)N(KL)N Non-radial g-mode Pulsator Ref.(KO)N. WD2132+096 See also (MR) WD2134+125 High gravity PG1159-like central star of NGC7094, type lgEH, Ref.(66) CSPN effective temperature 125,900K. (IO)N. WD2134+218 See also (PP)(NB) WD2136+229 See also (PP) WD2136+828 See also (NL) WD2137+102 See also (QJ)(NC) WD2138-332 See Also (NY)(OJ) See also (PV) WD2139+115 See also (PP) WD2140+207 Weak C2 reported, Ref.(5D) See also (PO)(OL)(NB)(JN)(OJ)(RQ) WD2142+004 See also (QJ) WD2142-169 See also (OR) WD2143+108 CPMB with WD 2143+108.1. Ref.(SK) WD2143+108.1 CMPB with WD 2143+108. Ref.(SK) WD2144+128 See also (NC) WD2144-004 See also (PY) WD2144-079 See also (QA)(PS)(OR) WD2146+005 See also (PD)(MV) WD2146+412 Reclassified as a helium strong sub-dwarf B star.(EG) The coolest known DBA white dwarf; TEFF= 12,500K, Ref.(62). WD2146-077 See also (PD)(MV) WD2147+280 G188-27 shows weak HeI; coolest DB? Ref.(CE). WD2148-075 DA; binary nature questionable.Ref.(QB) See also (QM) WD2148-291 Short period ZZ Ceti (OC) WD2149+000 See also (QJ)(NC) WD2149+002 See also (MV) WD2149+021 See also (QP)(QA)(PP)(MR)(NB)(NL) WD2149+126 See also (PD)(MV) WD2150+021 See also (PP) WD2150-008 Noisy spectrum; Ref.(QB)See also (NC) WD2151+125 Nearby bright star, binary nature questionable.; Ref.(QB) See also (QM) WD2151-015 Name(s) for MS companion(s). LTT 8747B See also (QP)(RO) WD2151-307 See also (RK) WD2152-310 ZZ Ceti candidate (HC) WD2152-548 See also (PP)(RK)(RK) WD2153-419 See also (PP)(JV)(RK) WD2154+408 WD2154+408 is a PCEB binary (P=0.26772 day) consisting of a hot white dwarf primary and a cool late MS companion. (HF) WD2154-437 See also (PR) WD2154-512 See also (OJ)(JV)(PR) WD2155-009 See also (NC) WD2157-074 See also (QJ)(NC) WD2157-079 See also (OW) WD2159-414 See also (PP) WD2159-754 See also (OJ) WD2200+113 See also (NC) WD2200-000 See also (QJ)(NC) WD2200-136 Double-lined double-degenerate binary. Ref.(PP) WD2201-005 See also (QJ)(NC) WD2202-282 ZZ Ceti candidate (HC) WD2203+005 See also (NC) WD2204-005 See also (QJ)(NC) WD2204-012 See also (NC) WD2205-015 WD+MS Eclipsing Binary System. Ref.(QN). WD2205-139 See also (PP) WD2206+121 See also (NC) WD2207+121 See also (RF)(RS) WD2207-004 See also (QJ)(NC) WD2207-303 See also (NL)(RK) WD2209-147 Double-lined double-degenerate binary. Ref.(PP) See also (QX)(QX) WD2211+372 See also (PS)(MQ) WD2211-316 ZZ Ceti candidate (HC) WD2211-392 See also (OJ) WD2211-495 See also (MV) WD2212+656 The DA degenerate central star of IW2, Ref.(7U). WD2213+007 PCEB. Ref.(QH) See also (NC) WD2213+125 See also (QJ)(NC) WD2214+005 See also (QJ)(NC) WD2215+368 See also (OJ) WD2215+388 GD 401 is a DB degenerate with upper limit calcium and magnesium abundances, Ref.(49). See also (PS)(QA) WD2215-002 See also (PD)(MV) WD2216+158 Double-lined double-degenerate binary. Ref.(PP) WD2216+484 GD402 probable unresolved DA+DC system, Ref.(23). WD2216-000 See also (QJ)(NC) WD2216-657 L119-34, DZ star with rare carbon, Ref.(DE). See also (QA)(OV) WD2218+002 See also (QJ)(NC) WD2218+706 The DA central star of DEHT5, Ref.(7U). WD2220+124 See also (QJ)(NC) WD2220+133 See also (PP)(MY)(OK) WD2221-165 See also (QV)(MR) WD2223+130 See also (NC) WD2224-004 See also (NC) WD2224-009 See also (QJ) WD2224-344 See also (PR) WD2225+118 See also (RF)(RS) WD2226+139 See also (NC) WD2226-007 See also (QJ)(NC) WD2226-210 Hydrogen dominated CSPN Ref.(KL)(SM) WD2226-754 Wide CPM pair with WD2226-755 Ref. (FF) See also (PV) WD2226-755 Wide CPM pair with WD2226-754 Ref. (FF) See also (PV) WD2227-010 See also (QJ)(NC) WD2227-010.1 See also (NC) WD2228+126 See also (QJ)(NC) WD2229+235 See also (QV)(MR) WD2230+125 See also (NC) WD2230-125 See also (PP)(MR) WD2231-005 See also (NC) WD2232+009 See also (NC) WD2233+142 See also (NC) WD2234-095 See also (NC) WD2235-305 ZZ Ceti candidate (HC) WD2236+129 See also (RF)(RS) WD2237+000 CPMB with WD2237+000.1 (OM) WD2237+000.1 CPMB with WD2237+000 (OM) WD2237+143 See also (QJ)(NC) WD2237-365 This is NOT LHS 3841 = LP 984-76 = Lephm 1-4978 as reported elswhere as per J.Farhi private communication 9/29/09 Finding Chart) WD2238-098 PCEB. Ref.(QH) See also (QJ)(NC) WD2239+001 See also (NC) WD2240+125.1 A visual double DA binary, Ref.(2T). WD2240+125.2 A visual double DA binary, Ref.(2T). See also (PP) WD2240+217 Post-common envelope binary. Ref.(QB) WD2240-017 See also (PP) WD2241+009 See also (NC) WD2242-002 See also (NC) WD2244+030 = PG2244+031 Star A is the WD. Finding Chart see A5.12 in Ref.(LJ) WD2245+146 See also (PD)(MV) WD2246+120 Reported by Handler,G. 2001,MNRAS,323,L43 to be a pulsating DB White Dwarf of type V777Her WD2246+223 See also (OJ)(MY)(NB)(NL) WD2246-001 See also (NC) WD2246-105 See also (NC) WD2247+583 See also (RK) WD2248+293 See also (OJ)(NN) WD2249-105 See section A5.10 in Ref. (LJ). WD2250-093 See also (NC) WD2251-070 See also (QA)(PC)(OJ)(NN) WD2252-005 See also (NC) WD2253+054 Very weak spectrum, common proper motion pair. NOTE:Arizona Finding Chart points to 225553 +054530 See also(PR) WD2253-081 G156-64 common proper motion binary with BD-8 5980 (G6 dwarf) See also (NZ)(PQ) WD2254+126 ZZ Ceti star ref.(KA) See also (PP) WD2256+249 GD245 is a composite DA + dM pre-cataclysmic binary, Ref.(9V) See also (MY)(OH) WD2256+313 See also (PR) WD2257+162 Name(s) for MS companion(s). PG 2257+162B WD2257-073 DA + G5V binary, REF.(14). WD2258+134 See also (QJ)(NC) WD2258+155 See also (QC) WD2258+406 See also (PQ) WD2259+143 Hot/cold Table 1 temperatures ambigious. Ref.(PP) WD2300-008 See also (QJ)(NC) WD2301+762 See also (PR) WD2301-072.1 CPM with WD2301-072.2, Ref.(3A). WD2301-072.2 CPM with WD2301-072.1, Ref.(3A). WD2303+242 KR Peg is a ZZ CETI variable, Ref.(44). See also (PB) WD2303-005 See also (QJ) WD2304+251 White dwarf companion to the mild barium star 56 PEG; may have accretion disk, Ref.(9T). WD2306+124 See also (QC)(PP) WD2308+050 See also (PP) WD2309+006 See also (QJ)(NC) WD2309+007 See also (QJ)(NC) WD2309+105 See also (PP)(JV)(MZ)(NL)(RX)(RK) WD2309-009 See also (RS) WD2310+005 See also (NC) WD2312-024 See also (QA) WD2313-313 ZZ Ceti candidate (HC) WD2315+003 See also (NC) WD2315-098 PCEB. Ref.(QH) See also (QJ)(NC) WD2316+123 New magnetic degenerate, with a 30Mg field, Ref.(5U). WD2316-011 See also (NC) WD2316-064 See also (PF)(MW)(NN) WD2316-098 See also (QJ)(NC) WD2316-173 IUE detection of CaII 1840A, Ref.(4L); strong UV CI lines, Ref.(CK). WD2317+008 See also (PD)(MV) WD2317+268 Name(s) for MS companion(s). KUV 23176+2650B WD2317-295 ZZ Ceti candidate (HC) WD2318+007.1 CPMB with WD 2318+007.2 Ref.(QL). WD2318+007.2 CPMB with WD 2318+007.1 Ref.(QL). WD2318+009 See also (NC) WD2318+126 See also (PP) WD2319+691.1 = A on Finding chart for GD 559B Ref.(LJ) WD2319+691.2 = B on Finding chart for GD 559B Ref.(LJ) WD2319-012 See also (QJ)(NC) WD2320+003 See also (PD)(MV) WD2321+005 See also (NC) WD2321-010 See also (MV) WD2321-549 See also (QM)(PP)(JV)(RK) WD2322+118 See also (OR) WD2322+137 See also (OJ) WD2322-011.1 See also (NC) WD2322-097 See also (QJ)(NC) WD2322-181 See also (PP) WD2323+157.2 Atmosphere virtually devoid of Hydrogen; Coolest known He atmosphere WD; Teff~3650K; Common proper motion pair with WD2323+157.1 (GD) Authors have witdrawn this paper. Star is a background subdwarf K7/M0 see A3.1 Ref.(LJ) see http://xxx.lan WD2323-006 See also (NC) WD2323-014 See also (NC) WD2324+397 Peculiar PG1159-like degenerate star of type lgEH, Ref.(66) Non-radial g-mode pulsator Ref.(KO)N. WD2326+049 G029-038 is a ZZ CETI variable, Ref.(AE)(JE)(MR), Contains circumstellar dust (NG) See also (QV)(QD)(QA)(PP)(PB)(OR)(OH)(NL)(OJ) WD2326-001 See also (NC) WD2326-004 See also (NC) WD2327+537 MS+MS superposition; Ref.(QB) WD2328+107 See also (PP) WD2329+134 See also (NC) WD2329+267 See also (MV) WD2329-090 See also (QJ)(NC) WD2330-212 Single-lined double-degenerate binary. Ref.(PP) WD2330-296 ZZ Ceti candidate (HC) WD2331+290 Newly identified double degenerate close binary, Ref.(7G). WD2331-005 See also (NC) WD2331-475 See also (MV)(NB)(NL) WD2333+301 WD associated with PN; Type: E Ref.(KL) WD2333-007 See also (NC) WD2333-049 See also (PS)(PP) WD2334-139 See also (PP) WD2335+305 JN1 is a PG1159 star with no detected variability and an associated planetary nebula, Ref.(DI); type E, Ref.(66). WD2335-002 See also (NC) WD2336-003 See also (QJ) WD2336-005 See also (QJ)(NC) WD2336-006 PCEB. Ref.(QH) See also (QJ)(NC) WD2336-079 Long period ZZ Ceti (OC) See also (OJ) WD2336-187 Double-lined double-degenerate binary. Ref.(PP) WD2337-760 Double-degenerate candidate Ref.(KP). WD2338+003 Post-common envelope binary. Ref.(QB) See also (QM) WD2339+157 See also (QJ)(NC) WD2339-100 See also (QJ)(NC) WD2340+154 See also (QJ) WD2341+322 EG162 common proper motion binary with G130-6 (M3 dwarf) See also (PV)(NL)(OJ)(PR) WD2342+001 See also (QJ) WD2342+806 GD561, the DAO central star of a newly discovered planetary nebula, Ref.(7T). WD2343+386 See also (PD)(MV) WD2343-005 Post-common envelope binary. Ref.(QB) See also (QM) WD2343-008 See also (NC) WD2343-106 See also (PD)(MV) WD2343-176 See also (PP) WD2344+434 See also (QJ) WD2344-006 See also (QJ)(NC) WD2344-266 See also (PR) WD2345-089 See also (NC) WD2345-313 ZZ Ceti candidate (HC) WD2345-396 See also (PP) WD2345-481 Single-lined double-degenerate binary. Ref.(PP) WD2347+004 See also (QJ) WD2347+128 ZZ Ceti star ref.(KA) See also (PP) WD2347+292 See also (OJ) WD2348-011 ZZ Ceti star Ref.(KB) WD2348-244 EC23487-2424 is a ZZ CETI variable, Ref.(44). See also (PP)(PB) WD2349+286 See also (NL) WD2349-283 See also (PP)(MQ) WD2349-364 See also (PP) WD2350+001 See also (OY) WD2350-083 The finding Charts place this star at 23 53 27.6 -8 4 41(2000) near the position of G273-B1A not G273-B1B. See also (PP)(PQ) WD2350-248 See also (PP) WD2350-279 ZZ Ceti candidate (HC) WD2351+650.1 CPM WD component with M > 15.0, REF.(3A). WD2351+650.2 CPM WD component with M > 15.0, REF.(3A). WD2351-335 Triple system DA5.5+dM3.5+dM8 see A5.3 in Ref.(LJ) See also (OJ)(PQ)(PR)(RO) WD2351-368 See also (PP)(MV) WD2352+401 G171-027 has weak C2, Ref.(CE). WD2354+159 See also (QA)(PS)(OR) WD2354-151 See also (PP) WD2357+296 See also (NL) WD2359-324 See also (PP) WD2359-434 See also (PP)(OJ)(NB)(OL) WD1159-034 See also (SM)