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## (from tabmap V6.0 (2016-08-18)) 2024-04-19T11:41:06 #--------------------------------------------------------------------------- #-- J/AJ/124/1670 Post-T Tauri Stars in Sco-Cen Association (Mamajek+, 2002) #-------------------------------------------------------------------------- #---Table: J/AJ/124/1670/./notes.dat Notes (55 records) # Note A1 --- [a-x] Note number # --- A1 --- [:] # Text A67 --- Text of note --------------------------------------------------------------------- N o t e Text --------------------------------------------------------------------- a:SIMBAD lists as variable or suspected variable, but Hipparcos a finds scatter in Hp<=0.015mag. The typical scatter for the other a standard stars was 0.005 mag in Hp (Hipparcos magnitude), with a none greater than 0.01mag. b:Spectroscopic binary. c:From standard list of Garcia (1989, Cat. <III/149>) and originally c in Johnson & Morgan (1953ApJ...117..313J), but not listed in c either Keenan & Yorka (1988BICDS..35...37K) or c Keenan & McNeil (1989, Cat. <III/150>). d:HR 5409 is a resolved binary (separation of 5") listed by SIMBAD d as a variable star, but Hipparcos found the scatter in the Hp d band to be only 0.015mag. e:HR 5072 is the planet host 70 Vir. Keenan & McNeil (1989, e Cat. <III/150>) call it G4 V, however it is G5 V in virtually e every other reference (e.g., Gray, Graham & Hoyt, e 2001AJ....121.2159G). We retain Keenan's classification f:Hipparcos "G" binary. g:CCDM J12165-5009AB. Unresolved binary ({rho}=0.2") h:The Michigan Spectral Survey (Houk, 1978, <III/51>) classifies h this star as K0/2(V)+(G) (quality = 3). We found it to be much h earlier (G1.5) and note that the published b-y and B-V colors h support an early G classification. i:Star "E" of Soderblom, King, & Henry (1998AJ....116..396S) i high-resolution survey of active southern stars. It is the most i Li-rich of the very active stars in the Soderblom sample. We did i not resolve this tight, equal-brightness binary i ({rho}=0.2"; CCDM J13431-6908AB). j:CCDM J15304-3218AB. Both stars were on the slit ({rho}=1.5") k:[KWS97] Lupus 1 26 = CCDM J15450-3412AB. Binary is resolved k ({rho}=3.4") but both were on-slit. l:[KWS97] TTS 79 = CCDM J15450-3412AB. Unresolved binary ({rho}=0.2") m:Star #10 = HIP 59721 is a common proper motion pair ({rho}=24") m with HD 106444 = HIP 59716 (F5V, {pi}=9.92+/-2.53) n:Star #19 = Einstein Slew Survey source 1ES 1233-63.4 o:Star #23 = HD 311894 = 2E 1241.6-6315 = Eclipsing binary o discovered in The All Sky Automated Survey Pojmanski (1998, o Cat. <J/other/AcA/48.35>): ASAS J124435-6331.8 (Per = 2.6 days) p:Star #27 = 2E 1255.1-7012 = EUVE J1258-70.4 q:Star #34 = PDS 66 = Hen 3-892 = IRAS 13185-6922. This is the q lone classical T Tauri star identified in this survey. q [O I] {lambda}6300 is seen in emission (EW = 0.2{AA}). r:Star #46 = CCDM J1437-4145AB. Unresolved binary ({rho} =0.4") s:Young ROSAT star identified by Wichmann et al. s (1997A&A...326..211W) t:Young ROSAT star identified by Krautter et al. t (1997, Cat. <J/A+AS/123/329>) v:Star #69 = CCDM J15394-2710AB. Unresolved binary ({rho}=0.4"). w:Star #76 = CCDM J16038-4356AB. Unresolved binary ({rho}=0.3"). x:Star #79. Faint companion off-slit ({rho}~=4"). u:Star #66 = CCDM J15370-3127A = RX J1537.0-3136 = 2E 1533.9-3126? u Our spectrum is of the bright (V=10) primary; the BC components u (both V=13) are 4" away, and off-slit. v:Star #69 = CCDM J15394-2710AB. Unresolved binary ({rho}=0.4"). w:Star #76 = CCDM J16038-4356AB. Unresolved binary ({rho}=0.3"). x:Star #79. Faint companion off-slit ({rho}~=4"). ---------------------------------------------------------------------