#Table: cats/aliases/P/PK/table5.dat (http://cdsarc.cds.unistra.fr)
----------------------------------------------------------------------------------------------
               |                    |u|
               |                    |_|
               |                    |P|
               | R  R        D  D  D|o|
Name           |Ah Am  RAs  Ed Em Es|s|Text
---------------|--------------------|-|-------------------------------------------------------
IRAS00170+6542 |00 17 05.7 +65 42 52| |Probably late AGB star (FC, Hrivnak etal.,1985).
IRAS00210+6221 |00 21 04.9 +62 21 39| |Probably late AGB star (FC, Hrivnak etal.,1985);
IRAS00210+6221 |00 21 04.9 +62 21 39| |  PPN (Hrivnak etal.,1999; Meixner etal.,1999).
IRAS00470+6429 |00 47 02.9 +64 29 16| |PPN candidate (Meixner etal.,1999).
IRAS01133+6434 |01 13 18.2 +64 34 54| |Probably late AGB star (FC, Hrivnak etal.,1985).
IRAS01144+6658 |01 14 26.3 +66 58 08| |AFGL 190. PPN candidate (Meixner etal.,1999).
IRAS01174+6110 |01 17 29.8 +61 10 35| |PPN (Hrivnak etal.,1999).
IRAS01304+6211 |01 30 27.6 +62 11 31| |OH 127.8+0.0. V 669 Cas. RAFGL 230. PPN cand.
IRAS01304+6211 |01 30 27.6 +62 11 31| |  (Meixner etal.,1999).
IRAS02143+5852 |02 14 22.0 +58 52 01| |PPN candidate (Meixner etal.,1999).
IRAS02152+2822 |02 15 12.5 +28 22 59| |PPN candidate (Meixner etal.,1999).
IRASZ02229+6208|02 22 53.0 +62 07 53| |In transition between AGB and PNe (Hrivnak etal.,
IRASZ02229+6208|02 22 53.0 +62 07 53| |  1997). Reflection nebulosity of PPN cand. (Ueta
IRASZ02229+6208|02 22 53.0 +62 07 53| |  etal.,1998). Carbon-rich PPN (Reddy etal.,1999).
IRAS02441+6922 |02 44 09.  +69 23 00| |Probably late AGB star (FC, Hrivnak etal.,1985).
HD 20041       |03 11 57.1 +56 57 22| |LSI+56 85. SAO 23903. PPN candidate (Meixner etal.,
HD 20041       |03 11 57.1 +56 57 22| |  1999).
IRAS04296+3429 |04 29 40.3 +34 29 53| |Likely between AGB and PNe (Kwok etal.,1989). See
IRAS04296+3429 |04 29 40.3 +34 29 53| |  Meixner etal.(1994); see Sahai (1999). Post-AGB
IRAS04296+3429 |04 29 40.3 +34 29 53| |  stage (FC, Reddy, Parthasarathy, 1996). Reflection
IRAS04296+3429 |04 29 40.3 +34 29 53| |  nebulosity of PPN cand. (Ueta etal.,1998).
IRAS04386+5722 |04 38 38.2 +57 22 11| |Stellar PPN cand. (Ueta etal.,1998). PPN candidate
IRAS04386+5722 |04 38 38.2 +57 22 11| |  (Meixner etal.,1999).
IRAS04505-1006 |04 50 35.3 -10 06 54| |Colour-selected PPN candidate (Volk, Kwok, 1989,
IRAS04505-1006 |04 50 35.3 -10 06 54| |  Table 4).
IRAS05089+0459 |05 08 56.6 +04 59 50| |PPN candidate (Meixner etal.,1999).
IRAS05113+1347 |05 11 18.1 +13 47 04| |PPN cand. (Kwok, 1993). Post-AGB stage (FC, Reddy,
IRAS05113+1347 |05 11 18.1 +13 47 04| |  Parthasarathy, 1996). Stellar PPN candidate (Ueta
IRAS05113+1347 |05 11 18.1 +13 47 04| |  etal.,1999).
IRAS05238-0626 |05 23 53.1 -06 26 29| |BD-06 1178. Most likely post-AGB supergiant evolving
IRAS05238-0626 |05 23 53.1 -06 26 29| |  towards PNe (FC, Reddy, Parthasarathy, 1996).
IRAS05341+0852 |05 34 10.1 +08 52 23| |Left AGB and becoming PN (Geballe,van der Veen,1990).
IRAS05341+0852 |05 34 10.1 +08 52 23| |  Post-AGB stage (FC, Reddy, Parthasarathy, 1996).Re-
IRAS05341+0852 |05 34 10.1 +08 52 23| |  flection nebulosity of PPN cand. (Ueta etal.,1998).
IRAS05381+1012 |05 38 11.0 +10 12 56| |PPN candidate (Kwok, 1993).
HD 44179       |06 17 37.0 -10 36 51| |Known as Red Rectangle. IRAS 06175-1036. BD-10 1476,
HD 44179       |06 17 37.0 -10 36 51| |  SAO 151362, a visual binary. Possible PPN (Bujar-
HD 44179       |06 17 37.0 -10 36 51| |  rabal etal.,1988; Jourdain de Muizon etal.,1990).
No.6-WSRT 2    |06 25 15.2 +12 48 56| |IRAS 06252+1248. IRAS-selected PN candidate; radio
No.6-WSRT 2    |06 25 15.2 +12 48 56| |  cont. data in WSRT 2 (Van de Steene, Pottasch,
No.6-WSRT 2    |06 25 15.2 +12 48 56| |  1995). FC, SECGPN (S1): VSP 4-6.
HD 46703       |06 33 49.3 +53 33 36| |SAO 25845. F supergiant as PPN candidate (Tamura
HD 46703       |06 33 49.3 +53 33 36| |  etal.,1993).
IRC -20101     |06 39 08.3 -22 13 47| |RAFGL 4521S. Possible pre-PN (Likkel etal.,1987).
IRAS06472-3713 |06 47 13.9 -37 13 08| |ST Pup. Colour-selected PPN candidate (Volk, Kwok,
IRAS06472-3713 |06 47 13.9 -37 13 08| |  1989, Table 3).
IRAS06530-0213 |06 53 00.9 -02 13 35| |PPN cand. (Kwok, 1993); see Hu etal. (1993a), No.21.
IRAS06530-0213 |06 53 00.9 -02 13 35| |  Post-AGB stage (FC, Reddy, Parthasarathy, 1996).Re-
IRAS06530-0213 |06 53 00.9 -02 13 35| |  flection nebulosity of PPN cand. (Ueta etal.,1998).
HD 51585       |06 55 37.6 +16 23 32| |Evolving towards early stage of PNe (Parthasarathy,
HD 51585       |06 55 37.6 +16 23 32| |  Pottasch, 1989).
IRAS07027-7934 |07 02 45.3 -79 34 23| |IR colours similar to that observed in PNe
IRAS07027-7934 |07 02 45.3 -79 34 23| |  (Parthasarathy, 1989). Probable [WC11] object
IRAS07027-7934 |07 02 45.3 -79 34 23| |  (FC, Menzies, Wolstencroft, 1990). Possible PPN
IRAS07027-7934 |07 02 45.3 -79 34 23| |  (Jourdain de Muizon etal.,1990).
IRAS07131-0147 |07 13 10.9 -01 47 23| |Polarized bipolar refl. nebula between AGB and PNe
IRAS07131-0147 |07 13 10.9 -01 47 23| |  (Scarrott etal.,1990).
IRAS07134+1005 |07 13 25.3 +10 05 09| |SAO 96709=HD 56126. Colour-selected PPN candidate
IRAS07134+1005 |07 13 25.3 +10 05 09| |  (Volk, Kwok, 1989, Table 3); likely between AGB
IRAS07134+1005 |07 13 25.3 +10 05 09| |  and PNe (Kwok etal.,1989). IR colours similar to
IRAS07134+1005 |07 13 25.3 +10 05 09| |  that observed in PNe (Parthasarathy, 1989).
IRAS07134+1005 |07 13 25.3 +10 05 09| |  Diffraction-limited images of the young carbon-rich
IRAS07134+1005 |07 13 25.3 +10 05 09| |  PPN (Dayal etal.,1995). Reflection nebulosity of
IRAS07134+1005 |07 13 25.3 +10 05 09| |  PPN candidate (Ueta etal.,1998).
IRAS07239-3325 |07 23 59.7 -33 25 19| |PPN candidate (Meixner etal.,1999).
IRAS07253-2001 |07 25 21.1 -20 01 08| |Most likely in post-AGB stage (FC, Reddy, Parthasa-
IRAS07253-2001 |07 25 21.1 -20 01 08| |  rathy, 1996).
IRAS07284-0940 |07 28 24.3 -09 40 15| |HD 59693. U Mon. SAO 134775. PPN candidate (Meixner
IRAS07284-0940 |07 28 24.3 -09 40 15| |  etal.,1999).
IRAS07331+0021 |07 33 07.1 +00 21 40| |AI CMi. Colour-selected PPN candidate (Volk, Kwok,
IRAS07331+0021 |07 33 07.1 +00 21 40| |  1989, Table 3).
OH 231.8+4.2   |07 39 58.9 -14 35 44| |QX Pup. IRAS 07399-1435. Known as Rotten Egg Nebula.
OH 231.8+4.2   |07 39 58.9 -14 35 44| |  Possible PPN (Bujarrabal etal.,1988). See Morris
OH 231.8+4.2   |07 39 58.9 -14 35 44| |  etal.(1987).
IRAS07430+1115 |07 43 04.2 +11 15 46| |In transition between AGB and PNe (Hrivnak etal.,
IRAS07430+1115 |07 43 04.2 +11 15 46| |  1997). Reflection neb. of PPN cand. (Ueta etal.,
IRAS07430+1115 |07 43 04.2 +11 15 46| |  1998). Carbon-rich PPN (Hrivnak, Kwok, 1999;
IRAS07430+1115 |07 43 04.2 +11 15 46| |  Reddy etal.,1999).
MWC 574        |07 45 44.8 -14 00 12| |Extremely-low-excitation object, may be PN in an
MWC 574        |07 45 44.8 -14 00 12| |  early stage of development (Sanduleak,
MWC 574        |07 45 44.8 -14 00 12| |  Stephenson, 1972). S1: Appendix to Table 1.
IRAS07536-2830 |07 53 38.4 -28 30 54| |HU Pup. SAO 174817. Intrinsically polarized object
IRAS07536-2830 |07 53 38.4 -28 30 54| |  in the transition from post-AGB to PN stage
IRAS07536-2830 |07 53 38.4 -28 30 54| |  (Trammell etal.,1994).
IRAS07582-4059 |07 58 14.4 -40 59 07| |PPN candidate (FC, Hu etal.,1993a, No.42).
IRAS08005-2356 |08 00 32.5 -23 56 16| |PPN associated with low-latitude F-type supergiant
IRAS08005-2356 |08 00 32.5 -23 56 16| |  (Slijkhuis etal.,1991); see Hu etal.(1993a),
IRAS08005-2356 |08 00 32.5 -23 56 16| |  No.27. OH 1612 MHz detected (Hu etal.,1994). Re-
IRAS08005-2356 |08 00 32.5 -23 56 16| |  flection nebulosity of PPN cand. (Ueta etal.,1998).
IRAS08143-4406 |08 14 23.1 -44 06 43| |Most likely in post-AGB stage (FC, Reddy, Parthasa-
IRAS08143-4406 |08 14 23.1 -44 06 43| |  rathy, 1996).
IRAS08187-1905 |08 18 42.6 -19 05 30| |HD 70379. Most likely post-AGB supergiant evolving
IRAS08187-1905 |08 18 42.6 -19 05 30| |  towards PNe (FC, Reddy, Parthasarathy, 1996).
IRAS09032-3953 |09 03 12.4 -39 53 10| |Colour-selected PPN candidate (Volk, Kwok, 1989,
IRAS09032-3953 |09 03 12.4 -39 53 10| |  Table 4); see Hu etal.(1993a), No.41.
IRAS09370-4826 |09 37 03.5 -48 26 34| |PPN candidate (FC, Hu etal.,1993a, No.47).
IRAS09371+1212 |09 37 12.0 +12 12 31| |Peculiar galaxy (FC, Condon, Broderick, 1986). Known
IRAS09371+1212 |09 37 12.0 +12 12 31| |  as Frosty Leo Nebula. Possible pre-PN (Likkel
IRAS09371+1212 |09 37 12.0 +12 12 31| |  etal.,1987). Evolved, mass-losing red giant,
IRAS09371+1212 |09 37 12.0 +12 12 31| |  post-AGB circumstellar envelope (FC, Forveille
IRAS09371+1212 |09 37 12.0 +12 12 31| |  etal.,1987). Possible PPN (Bujarrabal etal.,1988).
IRAS09371+1212 |09 37 12.0 +12 12 31| |  Pre-main-sequence young object? (Robinson etal.,
IRAS09371+1212 |09 37 12.0 +12 12 31| |  1992).
IRC +10216     |09 45 14.9 +13 30 41| |CW Leo. RAFGL 1381. A prob. PN progenitor (Zuckerman
IRC +10216     |09 45 14.9 +13 30 41| |  etal.,1976). See Skinner etal.(1998). Reflection
IRC +10216     |09 45 14.9 +13 30 41| |  nebulosity of PPN cand., IRAS 09452+1330 (Ueta etal.,
IRC +10216     |09 45 14.9 +13 30 41| |  1998). S1: Appendix to Table 1.
IRAS10029-5553 |10 02 54.6 -55 54 01| |PPN candidate (FC, Hu etal.,1993a, No.49). IRAS-radio
IRAS10029-5553 |10 02 54.6 -55 54 01| |  PN candidate (Van de Steene, Pottasch, 1993).
IRAS10131+3049 |10 13 10.7 +30 49 17| |RW LMi. RAFGL 1403. IRC +30219. PPN candidate
IRAS10131+3049 |10 13 10.7 +30 49 17| |  (Meixner etal.,1999).
IRC -10236     |10 14 34.5 -14 24 30| |IY Hya. Intrinsically polarized object in the tran-
IRC -10236     |10 14 34.5 -14 24 30| |  sition from post-AGB to PN stage (Trammell etal.,
IRC -10236     |10 14 34.5 -14 24 30| |  1994).
HD 89353       |10 15 49.9 -28 44 29| |AG Ant. IRAS 10158-2844. SAO 178644. HR 4049. Prob.
HD 89353       |10 15 49.9 -28 44 29| |  a low-mass star in a post-AGB (Waelkens, Waters,
HD 89353       |10 15 49.9 -28 44 29| |  1987). Intrinsically polarized object in the trans.
HD 89353       |10 15 49.9 -28 44 29| |  from post-AGB to PN stage (Trammell etal.,1994).
HD 89353       |10 15 49.9 -28 44 29| |  Stellar PPN candidate (Ueta etal.,1998).
IRAS10194-5625 |10 19 24.1 -56 25 23| |Colour-selected PPN candidate (Volk, Kwok, 1989,
IRAS10194-5625 |10 19 24.1 -56 25 23| |  Table 4); see Hu etal.(1993a), No.50.
IRAS10197-5750 |10 19 44.8 -57 50 32| |Known as Roberts 22, reflection nebula. AFGL 4104.
IRAS10197-5750 |10 19 44.8 -57 50 32| |  OH 284.18-0.79. IRAS 10197-5750. Colour-selected
IRAS10197-5750 |10 19 44.8 -57 50 32| |  PPN candidate (Volk, Kwok,1989, Table 4). CO obs.
IRAS10197-5750 |10 19 44.8 -57 50 32| |  of PPNe with bipolar structure (Bujarrabal,
IRAS10197-5750 |10 19 44.8 -57 50 32| |  Bachiler, 1991).
RAFGL 4106     |10 21 32.5 -59 16 54| |IRAS 10215-5916. IR colours similar to that observed
RAFGL 4106     |10 21 32.5 -59 16 54| |  in PNe (Parthasarathy, 1989). G-type supergiant in
RAFGL 4106     |10 21 32.5 -59 16 54| |  post-AGB stage (Garcia-Lario etal.,1994).
IRAS10481-6930 |10 48 08.8 -69 30 03| |Colour-selected PPN candidate (Volk, Kwok, 1989,
IRAS10481-6930 |10 48 08.8 -69 30 03| |  Table 4).
IRAS10491-2059 |10 49 11.3 -20 59 04| |V Hya. BD-20 3283. SAO 179278. IRC -20218. Intrin-
IRAS10491-2059 |10 49 11.3 -20 59 04| |  sically polarized object in the transition from
IRAS10491-2059 |10 49 11.3 -20 59 04| |  post-AGB to PN stage (Trammell etal.,1994).
IRAS11000-6153 |11 00 02.6 -61 53 33| |SAO 251227=HD 95767. PPN cand. (Volk, Kwok, 1989,
IRAS11000-6153 |11 00 02.6 -61 53 33| |  Table 1). FOIb star with far-IR excess and colours
IRAS11000-6153 |11 00 02.6 -61 53 33| |  similar to PNe (Pottasch, Parthasarathy, 1988).
IRAS11065-6026 |11 06 33.5 -60 26 35| |He 3-591. Colour-selected PPN candidate (Volk, Kwok,
IRAS11065-6026 |11 06 33.5 -60 26 35| |  1989, Table 4).
IRAS11339-6004 |11 33 59.9 -60 04 20| |PPN candidate (FC, Hu etal.,1993a, No.53).
IRAS11381-6401 |11 38 10.4 -64 01 49| |PPN candidate (FC, Hu etal.,1993a, No.60).
IRAS11385-5517 |11 38 33.7 -55 17 48| |SAO 239288=HD 101584=CP-54 4707. FOIape star with
IRAS11385-5517 |11 38 33.7 -55 17 48| |  far-IR excess (Parthasarathy, Pottasch, 1986);
IRAS11385-5517 |11 38 33.7 -55 17 48| |  PPN candidate (Volk, Kwok, 1989, Table 1).
IRAS11387-6113 |11 38 47.8 -61 13 51| |PPN candidate (FC, Hu etal.,1993a, No.55).
IRAS11472-0800 |11 47 15.2 -08 00 40| |PPN candidate (Meixner etal.,1999).
IRAS11544-6408 |11 54 26.1 -64 08 29| |PPN candidate (FC, Hu etal.,1993a, No.61).
1200-5333      |12 00 13.3 -53 33 24| |IRAS-radio PN candidate (Van de Steene, Pottasch,
1200-5333      |12 00 13.3 -53 33 24| |  1993).
CPD-53 5072    |12 17 33.3 -53 38 49| |IR colours similar to that observed in PNe
CPD-53 5072    |12 17 33.3 -53 38 49| |  (Parthasarathy, 1989).
IRAS12222-4652 |12 22 12.4 -46 52 30| |SAO 223420=HD 108015. PPN cand. (Volk, Kwok, 1989,
IRAS12222-4652 |12 22 12.4 -46 52 30| |  Table 1).F3Ib star with far-IR excess and colours
IRAS12222-4652 |12 22 12.4 -46 52 30| |  similar to PNe (Pottasch, Parthasarathy, 1988).
IRAS12262-6417 |12 26 13.6 -64 17 02| |Possible PN from near-IR obs. (Persi etal.,1993);
IRAS12262-6417 |12 26 13.6 -64 17 02| |  see Hu etal.(1993a), No.62.
IRAS12302-6317 |12 30 15.6 -63 17 06| |Possible PN from near-IR obs. (Persi etal.,1993).
IRAS12309-5928 |12 30 55.0 -59 28 45| |PPN candidate (FC, Hu etal.,1993a, No.51).
IRAS12323-2033 |12 32 19.1 -20 33 39| |RU Crv. BD-20 3674. SAO 180922. IRC -20241. Intrin-
IRAS12323-2033 |12 32 19.1 -20 33 39| |  sically polarized object in the transition from
IRAS12323-2033 |12 32 19.1 -20 33 39| |  post-AGB to PN stage (Trammell etal.,1994).
IRAS12358-6323 |12 35 53.2 -63 23 10| |PPN cand. (FC, Hu etal.,1993a, No.59). OH 1612 MHz
IRAS12358-6323 |12 35 53.2 -63 23 10| |  detected (Hu etal.,1994).
IRAS12359+0715 |12 35 57.6 +07 15 48| |R Vir. HD 109914. SAO 119509. IRC +10256. Intrin-
IRAS12359+0715 |12 35 57.6 +07 15 48| |  sically polarized object in the transition from
IRAS12359+0715 |12 35 57.6 +07 15 48| |  post-AGB to PN stage (Trammell etal.,1994).
1240-6219      |12 40 34.9 -62 19 48| |IRAS-radio PN candidate (Van de Steene, Pottasch,
1240-6219      |12 40 34.9 -62 19 48| |  1993).
ESO-172?07     |12 41 54.2 -54 14 47| |IRAS 12419-5414. Known as Boomerang Nebula, re-
ESO-172?07     |12 41 54.2 -54 14 47| |  flection nebula. CO obs. of PPNe (Bujarrabal,
ESO-172?07     |12 41 54.2 -54 14 47| |  Bachiler, 1991).
IRAS12447+0425 |12 44 45.6 +04 25 05| |RU Vir. BD+04 2651a=HD 111166. IRC +00224. Intrin-
IRAS12447+0425 |12 44 45.6 +04 25 05| |  sically polarized object in the transition from
IRAS12447+0425 |12 44 45.6 +04 25 05| |  post-AGB to PN stage (Trammell etal.,1994).
IRAS12538-2611 |12 53 48.6 -26 11 22| |HR 4912=HD 112374. PPN candidate (Volk, Kwok, 1989,
IRAS12538-2611 |12 53 48.6 -26 11 22| |  Table 1); see Luck etal.(1983).
IRAS13404-6059 |13 40 26.8 -60 59 41| |PPN candidate (FC, Hu etal.,1993a, No.54).
IRAS13416-6243 |13 41 36.6 -62 43 11| |Possibly in transition from AGB to PNe (van der Veen
IRAS13416-6243 |13 41 36.6 -62 43 11| |  etal.,1989a). See Hu etal.(1993a), No.58.
IRAS13428-6232 |13 42 49.6 -62 32 59| |Possibly in transition from AGB to PNe (van der Veen
IRAS13428-6232 |13 42 49.6 -62 32 59| |  etal.,1989a).
He 3-1013      |14 33 07.4 -64 35 01| |IRAS 14331-6435. CPD-64 2939. Evolving towards an
He 3-1013      |14 33 07.4 -64 35 01| |  early stage of PNe (Parthasarathy, Pottasch, 1989).
IRAS14341-6211 |14 34 10.2 -62 11 42| |PPN cand. (FC, Hu etal.,1993a, No.57). OH 1612 MHz
IRAS14341-6211 |14 34 10.2 -62 11 42| |  detected (Hu etal.,1994).
IRAS14429-4539 |14 42 55.2 -45 39 31| |PPN cand. (FC, Hu etal.,1993a, No.44). Most likely
IRAS14429-4539 |14 42 55.2 -45 39 31| |  in post-AGB stage (FC, Reddy, Parthasarathy, 1996).
IRAS14527-6204 |14 52 43.4 -62 04 49| |PPN candidate (FC, Hu etal.,1993a, No.56).
Hen 1044       |14 56 12.  -54 06 11| |He 2-113 (not a PN in CGPN). Between AGB and PNe
Hen 1044       |14 56 12.  -54 06 11| |  (Le Bertre etal.,1989). [WC11] object (Menzies,
Hen 1044       |14 56 12.  -54 06 11| |  Wolstencroft, 1990).
1510-5754      |15 10 25.2 -57 54 11| |IRAS-radio PN candidate (Van de Steene, Pottasch,
1510-5754      |15 10 25.2 -57 54 11| |  1993).
IRAS15255+1944 |15 25 32.2 +19 44 10| |WX Ser. IRC +20281. Intrinsically polarized object
IRAS15255+1944 |15 25 32.2 +19 44 10| |  in the transition from post-AGB to PN stage
IRAS15255+1944 |15 25 32.2 +19 44 10| |  (Trammell etal.,1994).
IRAS15373-5308 |15 37 22.7 -53 08 43| |Possibly in transition from AGB to PNe (van der Veen
IRAS15373-5308 |15 37 22.7 -53 08 43| |  etal.,1989a).
IRAS15373-4220 |15 37 22.9 -42 20 14| |Possibly in transition from AGB to PNe (van der Veen
IRAS15373-4220 |15 37 22.9 -42 20 14| |  etal.,1989a).
IRAS15405-4945 |15 40 32.1 -49 45 54| |OH 329.14+3.92. SiO maser in PPNe (Nyman etal.,
IRAS15405-4945 |15 40 32.1 -49 45 54| |  1998). See te Lintel Hekkert etal.(1988).
IRAS15452-5459 |15 45 17.1 -54 59 41| |Possibly in transition from AGB to PNe (van der Veen
IRAS15452-5459 |15 45 17.1 -54 59 41| |  etal.,1989a).
IRAS15465+2818 |15 46 31.7 +28 18 29| |R CrB. PPN candidate (Volk, Kwok, 1989, Table 1);
IRAS15465+2818 |15 46 31.7 +28 18 29| |  see Gillett etal.(1986). Stellar PPN candidate
IRAS15465+2818 |15 46 31.7 +28 18 29| |  (Ueta etal.,1998).
IRAS15532-4210 |15 53 16.3 -42 10 41| |SAO 226389=HD 142527=He 3-1119. F6IIIe star with
IRAS15532-4210 |15 53 16.3 -42 10 41| |  far-IR excess and colours similar to PNe (Pottasch,
IRAS15532-4210 |15 53 16.3 -42 10 41| |  Parthasarathy, 1988). PPN candidate (Volk, Kwok,
IRAS15532-4210 |15 53 16.3 -42 10 41| |  1989, Table 1).
IRAS15556-2248 |15 55 38.9 -22 48 42| |SAO 183986=HD 143006=He 3-1126. G5(I)e star with
IRAS15556-2248 |15 55 38.9 -22 48 42| |  far-IR excess and colours similar to PNe (Pottasch,
IRAS15556-2248 |15 55 38.9 -22 48 42| |  Parthasarathy, 1988). PPN candidate (Volk, Kwok,
IRAS15556-2248 |15 55 38.9 -22 48 42| |  1989, Table 1).
IRAS16029-4101 |16 02 59.4 -41 01 52| |PPN candidate (FC, Hu etal.,1993a, No.43).
IRAS16032-3537 |16 03 12.2 -35 37 19| |IRAS PSC PN candidate (F Carballo etal.,1992).
HD 144432      |16 03 53.6 -27 35 08| |SAO 184124=He 3-1141. FOIIIe star with far-IR excess
HD 144432      |16 03 53.6 -27 35 08| |  and colours similar to PNe (Pottasch,Parthasarathy,
HD 144432      |16 03 53.6 -27 35 08| |  1988).
IRAS16086-5255 |16 08 37.4 -52 55 44| |PPN candidate (FC, Hu etal.,1993a, No.48).
IRAS16115-5044 |16 11 31.1 -50 44 53| |Possibly in transition from AGB to PN (van der Veen
IRAS16115-5044 |16 11 31.1 -50 44 53| |  etal.,1989a).
IRAS16130-4620 |16 13 06.3 -46 20 36| |PPN candidate (FC, Hu etal.,1993a, No.45).
CPD-59 6723    |16 20 40.5 -59 56 38| |IR colours similar to that observed in PNe (Partha-
CPD-59 6723    |16 20 40.5 -59 56 38| |  sarathy, 1989).
Hen 1191       |16 23 31.0 -48 32 46| |IRAS 16235-4832. Bipolar nebula in stage between
Hen 1191       |16 23 31.0 -48 32 46| |  AGB and PNe (FC, Le Bertre etal.,1989).
IRC +30292     |16 26 00.6 +34 54 45| |V 697 Her. IRAS 16260+3454. Intrinsically polarized
IRC +30292     |16 26 00.6 +34 54 45| |  object in the transition from post-AGB to PNe stage
IRC +30292     |16 26 00.6 +34 54 45| |  (Trammell etal.,1994).
IRAS16275-2638 |16 27 32.2 -26 38 27| |Colour-selected PPN candidate (Volk, Kwok, 1989,
IRAS16275-2638 |16 27 32.2 -26 38 27| |  Table 4).
IRAS16279-4757 |16 27 56.4 -47 57 43| |Possibly in transition from AGB to PNe (van der Veen
IRAS16279-4757 |16 27 56.4 -47 57 43| |  etal.,1989a). See Hu etal.(1993a), No.46.
1633-4807      |16 33 23.4 -48 07 40| |IRAS-radio PN candidate (Van de Steene, Pottasch,
1633-4807      |16 33 23.4 -48 07 40| |  1993).
IRAS16342-3814 |16 34 17.1 -38 14 18| |Known as Water-Fountain Nebula. IR colours similar to
IRAS16342-3814 |16 34 17.1 -38 14 18| |  that observed in PNe (Parthasarathy, 1989).Reflect-
IRAS16342-3814 |16 34 17.1 -38 14 18| |  ion nebulosity of PPN cand. (Ueta etal.,1998).
IRAS16342-3814 |16 34 17.1 -38 14 18| |  Post-AGB class. (Sahai etal.,1999).
IRAS16399-6247 |16 39 58.8 -62 47 52| |SAO 253680=-62 5428. F2 star with far-IR excess and
IRAS16399-6247 |16 39 58.8 -62 47 52| |  colours similar to PNe (Pottasch, Parthasarathy,
IRAS16399-6247 |16 39 58.8 -62 47 52| |  1988).
IRAS16434-2244 |16 43 28.9 -22 44 19| |PN-colour IRAS source ass. with radio cont. source
IRAS16434-2244 |16 43 28.9 -22 44 19| |  (Ratag, Pottasch, 1991).
IRAS16552-3050 |16 55 16.5 -30 50 37| |PPN candidate (FC, Hu etal.,1993a, No.35).
IRAS16559-2957 |16 55 57.4 -29 57 09| |PPN cand. (FC, Hu etal.,1993a, No.34). OH 1612 MHz
IRAS16559-2957 |16 55 57.4 -29 57 09| |  detected (Hu etal.,1994).
IRAS16581-2039 |16 58 11.0 -20 39 53| |PN-colour IRAS source ass. with radio cont. source
IRAS16581-2039 |16 58 11.0 -20 39 53| |  (Ratag, Pottasch, 1991).
IRAS16582-1919 |16 58 18.6 -19 20 29| |PN-colour IRAS source ass. with radio cont. source
IRAS16582-1919 |16 58 18.6 -19 20 29| |  (Ratag, Pottasch, 1991).
IRAS17074-4549 |17 07 25.8 -45 49 16| |Possibly in transition from AGB to PNe (van der Veen
IRAS17074-4549 |17 07 25.8 -45 49 16| |  etal.,1989a).
IRAS17079-3926 |17 07 57.9 -39 26 15| |PN-colour IRAS source ass. with radio cont. source
IRAS17079-3926 |17 07 57.9 -39 26 15| |  (Ratag etal.,1990, No.3).
IRAS17086-2403 |17 08 40.2 -24 03 48| |PN-colour IRAS source ass. with radio cont. source
IRAS17086-2403 |17 08 40.2 -24 03 48| |  (Ratag, Pottasch, 1991). Most likely post-AGB
IRAS17086-2403 |17 08 40.2 -24 03 48| |  supergiant evolving towards PNe (Reddy, Parthasa-
IRAS17086-2403 |17 08 40.2 -24 03 48| |  rathy, 1996).
IRAS17088-4221 |17 08 48.2 -42 21 34| |Possibly in transition from AGB to PNe (van der Veen
IRAS17088-4221 |17 08 48.2 -42 21 34| |  etal.,1989a).
IRAS17092-3539 |17 09 13.4 -35 39 44| |PN-colour IRAS source ass. with radio cont. source
IRAS17092-3539 |17 09 13.4 -35 39 44| |  (Ratag etal.,1990, No.5).
IRAS17097-3210 |17 09 43.8 -32 11 02| |Possibly in transition from AGB to PNe (van der Veen
IRAS17097-3210 |17 09 43.8 -32 11 02| |  etal.,1989a).
IRAS17103-3338 |17 10 18.5 -33 39 45| |PN-colour IRAS source ass. with radio cont. source
IRAS17103-3338 |17 10 18.5 -33 39 45| |  (Ratag etal.,1990, No.6).
IRAS17106-3046 |17 10 38.9 -30 46 13| |PPN (Hrivnak etal.,1999). PPN candidate (Meixner
IRAS17106-3046 |17 10 38.9 -30 46 13| |  etal.,1999).
IRAS17111-2328 |17 11 06.7 -23 28 01| |PN-colour IRAS source ass. with radio cont. source
IRAS17111-2328 |17 11 06.7 -23 28 01| |  (Ratag, Pottasch, 1991).
IRAS17112-1918 |17 11 10.7 -19 18 45| |PN-colour IRAS source ass. with radio cont. source
IRAS17112-1918 |17 11 10.7 -19 18 45| |  (Ratag, Pottasch, 1991).
IRAS17114-3532 |17 11 29.2 -35 32 16| |PN-colour IRAS source ass. with radio cont. source
IRAS17114-3532 |17 11 29.2 -35 32 16| |  (Ratag etal.,1990, No.7).
IRAS17123-3929 |17 12 23.9 -39 29 49| |PN-colour IRAS source ass. with radio cont. source
IRAS17123-3929 |17 12 23.9 -39 29 49| |  (Ratag etal.,1990, No.8).
IRAS17125-3507 |17 12 28.7 -35 07 15| |PN-colour IRAS source ass. with radio cont. source
IRAS17125-3507 |17 12 28.7 -35 07 15| |  (Ratag etal.,1990, No.9).
IRAS17127-2428 |17 12 41.3 -24 27 55| |PN-colour IRAS source ass. with radio cont. source
IRAS17127-2428 |17 12 41.3 -24 27 55| |  (Ratag, Pottasch, 1991).
IRAS17131-3330 |17 13 09.0 -33 30 08| |PN-colour IRAS source ass. with radio cont. source
IRAS17131-3330 |17 13 09.0 -33 30 08| |  (Ratag etal.,1990, No.10).
IRAS17135-2748 |17 13 28.1 -27 48 26| |PN-colour IRAS source ass. with radio cont. source
IRAS17135-2748 |17 13 28.1 -27 48 26| |  (Ratag etal.,1990, No.46).
IRAS17149-3053 |17 14 52.1 -30 53 07| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17149-3053 |17 14 52.1 -30 53 07| |  1988, No.17). See Hu etal.(1993a), No.36 -coordi-
IRAS17149-3053 |17 14 52.1 -30 53 07| |  nates different. OH 1612 MHz detected (Hu etal.,
IRAS17149-3053 |17 14 52.1 -30 53 07| |  1994).
OH 349.2-0.2   |17 15 04.0 -37 54 54| |OH 349.36-020. IRAS 17150-3754. In transition phase
OH 349.2-0.2   |17 15 04.0 -37 54 54| |  between OH/IR star and PN (Pottasch etal.,1987).
IRAS17150-3224 |17 15 04.6 -32 24 15| |RAFGL 6815. IR colours similar to that observed in
IRAS17150-3224 |17 15 04.6 -32 24 15| |  PNe (Parthasarathy, 1989). See Hu etal.(1993a),
IRAS17150-3224 |17 15 04.6 -32 24 15| |  No.38. G2I, bipolar reflection nebula, young PPN
IRAS17150-3224 |17 15 04.6 -32 24 15| |  (Hu etal.,1993b). OH 1612 MHz detected (Hu etal.,
IRAS17150-3224 |17 15 04.6 -32 24 15| |  1994). Post-AGB stage (FC, Reddy, Parthasarathy,
IRAS17150-3224 |17 15 04.6 -32 24 15| |  1996). Reflection nebulosity of PPN cand. (Ueta
IRAS17150-3224 |17 15 04.6 -32 24 15| |  etal.,1999).
IRAS17153-3814 |17 15 16.6 -38 13 44| |PN-colour IRAS source ass. with radio cont. source
IRAS17153-3814 |17 15 16.6 -38 13 44| |  (Ratag etal.,1990, No.11).
Hen 1379       |17 16 21.3 -39 07 35| |IRAS 17163-3907. Point source in stage between AGB
Hen 1379       |17 16 21.3 -39 07 35| |  and PNe (Le Bertre etal.,1989).
IRAS17169-2528 |17 16 57.4 -25 28 31| |PN-colour IRAS source ass. with radio cont. source
IRAS17169-2528 |17 16 57.4 -25 28 31| |  (Ratag, Pottasch, 1991).
IRAS17178-2600 |17 17 48.4 -26 00 00| |PN-colour IRAS source ass. with radio cont. source
IRAS17178-2600 |17 17 48.4 -26 00 00| |  (Ratag, Pottasch, 1991).
IRAS17194-3137 |17 19 26.5 -31 37 05| |PN-colour IRAS source ass. with radio cont. source
IRAS17194-3137 |17 19 26.5 -31 37 05| |  (Ratag etal.,1990, No.13).
IRAS17195-2710 |17 19 35.9 -27 10 48| |Heavily-reddened low-exc. em.-line object (FC, Hu
IRAS17195-2710 |17 19 35.9 -27 10 48| |  etal.,1993a, No.31). SECGPN (S1): GLMP 554.
IRAS17207-2856 |17 20 44.7 -28 55 53| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17207-2856 |17 20 44.7 -28 55 53| |  1988, No.2).
IRAS17208-3859 |17 20 52.3 -38 59 03| |PN-colour IRAS source ass. with radio cont. source
IRAS17208-3859 |17 20 52.3 -38 59 03| |  (Ratag etal.,1990, No.14).
IRAS17217-3040 |17 21 45.4 -30 40 24| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17217-3040 |17 21 45.4 -30 40 24| |  1988, No.3).
IRAS17230-1832 |17 23 04.9 -18 32 15| |PN-colour IRAS source ass. with radio cont. source
IRAS17230-1832 |17 23 04.9 -18 32 15| |  (Ratag, Pottasch, 1991).
IRAS17230-3042 |17 23 10.5 -30 43 06| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17230-3042 |17 23 10.5 -30 43 06| |  1988, No.18).
IRAS17233-2602 |17 23 22.6 -26 02 25| |PPN candidate (F, Hu etal.,1993, No.30). OH 0.1+5.1
IRAS17233-2602 |17 23 22.6 -26 02 25| |  (Hu etal.,1994).
IRAS17234-4008 |17 23 29.0 -40 08 40| |PN-colour IRAS source ass. with radio cont. source
IRAS17234-4008 |17 23 29.0 -40 08 40| |  (Ratag etal.,1990, No.16).
IRAS17235-3400 |17 23 37.3 -34 00 36| |PN-colour IRAS source ass. with radio cont. source
IRAS17235-3400 |17 23 37.3 -34 00 36| |  (Ratag etal.,1990, No.17).
IRAS17237-3359 |17 23 44.9 -33 59 17| |PN-colour IRAS source ass. with radio cont. source
IRAS17237-3359 |17 23 44.9 -33 59 17| |  (Ratag etal.,1990, No.18).
IRAS17245-2519 |17 24 33.5 -25 19 57| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17245-2519 |17 24 33.5 -25 19 57| |  1988, No.5). PPN (Hrivnak etal.,1999).
IRAS17245-3951 |17 24 35.6 -39 51 17| |Colour-selected PPN candidate (Volk, Kwok, 1989,
IRAS17245-3951 |17 24 35.6 -39 51 17| |  Table 4). Bipolar PPN (Hrivnak etal.,1999).
IRAS17249-3703 |17 24 57.5 -37 03 05| |PN-colour IRAS source ass. with radio cont. source
IRAS17249-3703 |17 24 57.5 -37 03 05| |  (Ratag etal.,1990, No.19).
IRAS17277-3506 |17 27 43.6 -35 06 37| |HD 319896=-35 11646=He 3-1418. F8e star with far-IR
IRAS17277-3506 |17 27 43.6 -35 06 37| |  excess and colours similar to PNe (Pottasch,
IRAS17277-3506 |17 27 43.6 -35 06 37| |  Parthasarathy, 1988). PPN cand. (Volk, Kwok, 1989,
IRAS17277-3506 |17 27 43.6 -35 06 37| |  Table 1).
IRAS17281-3100 |17 28 08.7 -31 00 00| |PN-colour IRAS source ass. with radio cont. source
IRAS17281-3100 |17 28 08.7 -31 00 00| |  (Ratag, Pottasch, 1991).
IRAS17291-2402 |17 29 11.9 -24 02 45| |PN-colour IRAS source ass. with radio cont. source
IRAS17291-2402 |17 29 11.9 -24 02 45| |  (Ratag, Pottasch, 1991). Post-AGB stage (FC,Reddy,
IRAS17291-2402 |17 29 11.9 -24 02 45| |  Parthasarathy, 1996).
IRAS17300-3509 |17 30 02.1 -35 09 00| |PN-colour IRAS source ass. with radio cont. source
IRAS17300-3509 |17 30 02.1 -35 09 00| |  (Ratag etal.,1990, No.23).
IRAS17301-2538 |17 30 07.6 -25 38 21| |PN-colour IRAS source ass. with radio cont. source
IRAS17301-2538 |17 30 07.6 -25 38 21| |  (Ratag, Pottasch, 1991).
IRAS17307-1739 |17 30 39.0 -17 38 51| |PN-colour IRAS source ass. with radio cont. source
IRAS17307-1739 |17 30 39.0 -17 38 51| |  (Ratag, Pottasch, 1991).
IRAS17311-4924 |17 31 11.2 -49 24 25| |He 3-1428. Possibly in transition from AGB to PNe
IRAS17311-4924 |17 31 11.2 -49 24 25| |  (van der Veen etal.,1989a).
IRAS17318-2739 |17 31 50.0 -27 39 18| |PN-colour IRAS source ass. with radio cont. source
IRAS17318-2739 |17 31 50.0 -27 39 18| |  (Ratag, Pottasch, 1991).
IRAS17319-2521 |17 31 57.0 -25 21 55| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17319-2521 |17 31 57.0 -25 21 55| |  1988, No.21). PN-colour IRAS source ass. with
IRAS17319-2521 |17 31 57.0 -25 21 55| |  radio cont. source (Ratag etal.,1990, No.24).
IRAS17320-2043 |17 31 59.9 -20 43 37| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17320-2043 |17 31 59.9 -20 43 37| |  1988, No.22).
IRAS17323-2424 |17 32 20.0 -24 23 59| |PN-colour IRAS source ass. with radio cont. source
IRAS17323-2424 |17 32 20.0 -24 23 59| |  (Ratag, Pottasch, 1991).
IRAS17324-2805 |17 32 26.8 -28 06 13| |PN-colour IRAS source ass. with radio cont. source
IRAS17324-2805 |17 32 26.8 -28 06 13| |  (Ratag etal.,1990, No.25).
IRAS17330-3250 |17 33 03.8 -32 50 47| |PN-colour IRAS source ass. with radio cont. source
IRAS17330-3250 |17 33 03.8 -32 50 47| |  (Ratag etal.,1990, No.26).
IRAS17330-3441 |17 33 04.1 -34 42 40| |PN-colour IRAS source ass. with radio cont. source
IRAS17330-3441 |17 33 04.1 -34 42 40| |  (Ratag etal.,1990, No.27).
IRAS17332-2451 |17 33 15.7 -24 50 31| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17332-2451 |17 33 15.7 -24 50 31| |  1988, No.23).
IRAS17333-1731 |17 33 21.7 -17 31 11| |PN-colour IRAS source ass. with radio cont. source
IRAS17333-1731 |17 33 21.7 -17 31 11| |  (Ratag, Pottasch, 1991).
IRAS17347-3139 |17 34 45.9 -31 39 11| |PN-colour IRAS source ass. with radio cont. source
IRAS17347-3139 |17 34 45.9 -31 39 11| |  (Ratag etal.,1990, No.28).
IRAS17347-2519 |17 34 46.0 -25 19 01| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17347-2519 |17 34 46.0 -25 19 01| |  1988, No.24).
IRAS17350-2718 |17 34 59.3 -27 18 32| |PN-colour IRAS source ass. with radio cont. source
IRAS17350-2718 |17 34 59.3 -27 18 32| |  (Ratag etal.,1990, No.29).
IRAS17361-2358 |17 36 15.2 -23 57 43| |PN-colour IRAS source ass. with radio cont. source
IRAS17361-2358 |17 36 15.2 -23 57 43| |  (Ratag, Pottasch, 1991).
IRAS17368-3017 |17 36 51.0 -30 17 32| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17368-3017 |17 36 51.0 -30 17 32| |  1988, No.7).
IRAS17369-2329 |17 36 57.2 -23 29 20| |PN-colour IRAS source ass. with radio cont. source
IRAS17369-2329 |17 36 57.2 -23 29 20| |  (Ratag, Pottasch, 1991).
IRAS17374-3013 |17 37 21.2 -30 14 11| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17374-3013 |17 37 21.2 -30 14 11| |  1988, No.8).
IRAS17374-2840 |17 37 24.8 -28 40 09| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17374-2840 |17 37 24.8 -28 40 09| |  1988, No.25).
IRAS17374-2426 |17 37 25.2 -24 26 09| |PN-colour IRAS source ass. with radio cont. source
IRAS17374-2426 |17 37 25.2 -24 26 09| |  (Ratag, Pottasch, 1991).
IRAS17375-2759 |17 37 29.4 -27 59 29| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17375-2759 |17 37 29.4 -27 59 29| |  1988, No.26).
IRAS17375-3000 |17 37 32.4 -30 00 29| |PN-colour IRAS source ass. with radio cont. source
IRAS17375-3000 |17 37 32.4 -30 00 29| |  (Ratag etal.,1990, No.32).
IRAS17375-2742 |17 37 33.0 -27 42 08| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17375-2742 |17 37 33.0 -27 42 08| |  1988, No.27).
IRAS17381-3308 |17 38 11.0 -33 08 54| |PN-colour IRAS source ass. with radio cont. source
IRAS17381-3308 |17 38 11.0 -33 08 54| |  (Ratag etal.,1990, No.33).
IRAS17385-3332 |17 38 34.4 -33 32 14| |PPN cand. (FC, Hu etal.,1993a, No.39). OH 1612 MHz
IRAS17385-3332 |17 38 34.4 -33 32 14| |  detected (Hu etal.,1994).
IRAS17385-2613 |17 38 37.2 -26 13 04| |PN-colour IRAS source ass. with radio cont. source
IRAS17385-2613 |17 38 37.2 -26 13 04| |  (Ratag etal.,1990, No.47).
OH 0.9+1.3     |17 39 24.7 -27 27 02| |IRAS 17393-2727. In the transition phase between
OH 0.9+1.3     |17 39 24.7 -27 27 02| |  OH/IR stars and PNe (Pottasch etal.,1987).
IRAS17399-2136 |17 39 57.0 -21 36 51| |PN-colour IRAS source ass. with radio cont. source
IRAS17399-2136 |17 39 57.0 -21 36 51| |  (Ratag, Pottasch, 1991).
IRAS17400-3144 |17 40 00.9 -31 44 24| |PN-colour IRAS source ass. with radio cont. source
IRAS17400-3144 |17 40 00.9 -31 44 24| |  (Ratag etal.,1990, No.35).
IRAS17401-3052 |17 40 08.0 -30 52 36| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17401-3052 |17 40 08.0 -30 52 36| |  1988, No.9).
IRAS17403-2755 |17 40 28.5 -27 56 23| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17403-2755 |17 40 28.5 -27 56 23| |  1988, No.19).
IRAS17404-2713 |17 40 28.9 -27 13 18| |Possibly in transition from AGB to PN (van der Veen
IRAS17404-2713 |17 40 28.9 -27 13 18| |  etal.,1989a). PN-colour IRAS source ass. with
IRAS17404-2713 |17 40 28.9 -27 13 18| |  radio cont. source (Ratag, Pottasch, 1991).See Hu
IRAS17404-2713 |17 40 28.9 -27 13 18| |  etal.(1993a), No.32. OH 1.2+1.3 (Hu etal.,1994).
IRAS17412-2757 |17 41 10.8 -27 56 53| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17412-2757 |17 41 10.8 -27 56 53| |  1988, No.20).
IRAS17413-2719 |17 41 21.8 -27 19 26| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17413-2719 |17 41 21.8 -27 19 26| |  1988, No.10).
IRAS17415-2801 |17 41 33.6 -28 01 55| |PN-colour IRAS source ass. with radio cont. source
IRAS17415-2801 |17 41 33.6 -28 01 55| |  (Ratag, Pottasch, 1991).
IRAS17416-2755 |17 41 37.0 -27 55 10| |PN-colour IRAS source ass. with radio cont. source
IRAS17416-2755 |17 41 37.0 -27 55 10| |  (Ratag, Pottasch, 1991).
IRAS17418-2713 |17 41 51.9 -27 13 33| |PN-colour IRAS source ass. with radio cont. source
IRAS17418-2713 |17 41 51.9 -27 13 33| |  (Ratag, Pottasch, 1991).
IRAS17418-3335 |17 41 55.5 -33 35 32| |PN-colour IRAS source ass. with radio cont. source
IRAS17418-3335 |17 41 55.5 -33 35 32| |  (Ratag etal.,1990, No.37).
IRAS17422-2301 |17 42 14.4 -23 00 05| |PN-colour IRAS source ass. with radio cont. source
IRAS17422-2301 |17 42 14.4 -23 00 05| |  (Ratag, Pottasch, 1991).
IRAS17423-2943 |17 42 18.2 -29 43 35| |PN-colour IRAS source ass. with radio cont. source
IRAS17423-2943 |17 42 18.2 -29 43 35| |  (Ratag etal.,1990, No.48).
IRAS17424-2941 |17 42 29.0 -29 41 44| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17424-2941 |17 42 29.0 -29 41 44| |  1988, No.12).
IRAS17426-2508 |17 42 35.5 -25 08 03| |PN-colour IRAS source ass. with radio cont. source
IRAS17426-2508 |17 42 35.5 -25 08 03| |  (Ratag, Pottasch, 1991).
IRAS17428-2724 |17 42 53.4 -27 24 50| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17428-2724 |17 42 53.4 -27 24 50| |  1988, No.13).
IRAS17433-1750 |17 43 20.6 -17 50 36| |PPN cand. (FC, Hu etal.,1993a, No.24). OH 1612 MHz
IRAS17433-1750 |17 43 20.6 -17 50 36| |  detected (Hu etal.,1994).
IRAS17436-2702 |17 43 36.3 -27 02 19| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17436-2702 |17 43 36.3 -27 02 19| |  1988, No.14).
IRAS17436+5003 |17 43 41.3 +50 03 48| |SAO 30548=BD+50 2457=HD 161796. V 814 Her.RAFGL 5384.
IRAS17436+5003 |17 43 41.3 +50 03 48| |  F3Ib star with far-IR excess (Parthasarathy,
IRAS17436+5003 |17 43 41.3 +50 03 48| |  Pottasch, 1986). Possible PPN (Likkel etal.,1987).
IRAS17436+5003 |17 43 41.3 +50 03 48| |  PPN cand. (Hrivnak etal.,1989). Colour-selected
IRAS17436+5003 |17 43 41.3 +50 03 48| |  PPN candidate (Volk, Kwok, 1989, Table 1,3,4).
IRAS17436+5003 |17 43 41.3 +50 03 48| |  F supergiant as PPN cand. (Tamura etal.,1993);
IRAS17436+5003 |17 43 41.3 +50 03 48| |  see Hawkins etal. (1994). Reflection nebulosity
IRAS17436+5003 |17 43 41.3 +50 03 48| |  of PPN cand. (Ueta etal.,1998).
IRAS17437-3144 |17 43 46.3 -31 44 32| |PN-colour IRAS source ass. with radio cont. source
IRAS17437-3144 |17 43 46.3 -31 44 32| |  (Ratag etal.,1990, No.38).
IRAS17440-2321 |17 44 00.0 -23 19 56| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17440-2321 |17 44 00.0 -23 19 56| |  1988, No.28).
IRAS17440-3021 |17 44 00.7 -30 21 17| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17440-3021 |17 44 00.7 -30 21 17| |  1988, No.15).
IRAS17441-2411 |17 44 04.6 -24 11 57| |AFGL 5385. Possibly in transition from AGB to PN
IRAS17441-2411 |17 44 04.6 -24 11 57| |  (van der Veen etal.,1989a). Colour-selected PPN
IRAS17441-2411 |17 44 04.6 -24 11 57| |  candidate (Volk, Kwok, 1989, Table 4). PPN cand.
IRAS17441-2411 |17 44 04.6 -24 11 57| |  (Kwok, 1993). See Hu etal.(1993a), No.28.Post-AGB
IRAS17441-2411 |17 44 04.6 -24 11 57| |  stage (FC, Reddy, Parthasarathy, 1996).Reflection
IRAS17441-2411 |17 44 04.6 -24 11 57| |  nebulosity of PPN cand. (Ueta etal.,1998).
IRAS17443-2949 |17 44 23.8 -29 49 46| |PN-colour IRAS source ass. with radio cont. source
IRAS17443-2949 |17 44 23.8 -29 49 46| |  (Ratag etal.,1990, No.39).
IRAS17453-2503 |17 45 18.8 -25 03 44| |PN-colour IRAS source ass. with radio cont. source
IRAS17453-2503 |17 45 18.8 -25 03 44| |  (Ratag, Pottasch, 1991).
IRAS17456-2037 |17 45 41.5 -20 37 15| |PPN candidate (FC, Hu etal.,1993a, No.26).
IRAS17460-3114 |17 46 02.4 -31 14 21| |PN-colour IRAS source ass. with radio cont. source
IRAS17460-3114 |17 46 02.4 -31 14 21| |  (Ratag etal.,1990, No.40).
IRAS17461-3145 |17 46 12.1 -31 45 38| |PN-colour IRAS source ass. with radio cont. source
IRAS17461-3145 |17 46 12.1 -31 45 38| |  (Ratag etal.,1990, No.41).
IRAS17465-2350 |17 46 31.6 -23 50 23| |PN-colour IRAS source ass. with radio cont. source
IRAS17465-2350 |17 46 31.6 -23 50 23| |  (Ratag, Pottasch, 1991).
IRAS17466-2431 |17 46 35.5 -24 31 23| |PN-colour IRAS source ass. with radio cont. source
IRAS17466-2431 |17 46 35.5 -24 31 23| |  (Ratag, Pottasch, 1991).
IRAS17466-3031 |17 46 39.4 -30 32 10| |PN-colour IRAS source ass. with radio cont. source
IRAS17466-3031 |17 46 39.4 -30 32 10| |  (Ratag etal.,1990, No.42).
IRAS17474-2738 |17 47 26.5 -27 37 32| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17474-2738 |17 47 26.5 -27 37 32| |  1988, No.30).
IRAS17477-2452 |17 47 41.7 -24 51 44| |PN-colour IRAS source ass. with radio cont. source
IRAS17477-2452 |17 47 41.7 -24 51 44| |  (Ratag, Pottasch, 1991).
IRAS17487-1922 |17 48 47.2 -19 22 58| |Possibly in transition from AGB to PN (van der Veen
IRAS17487-1922 |17 48 47.2 -19 22 58| |  etal.,1989a).
IRAS17497-2618 |17 49 46.8 -26 17 47| |PN-colour IRAS source ass. with radio cont. source
IRAS17497-2618 |17 49 46.8 -26 17 47| |  (Ratag, Pottasch, 1991).
IRAS17498-2526 |17 49 53.8 -25 26 45| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17498-2526 |17 49 53.8 -25 26 45| |  1988, No.31).
IRAS17500-2405 |17 50 05.5 -24 04 48| |PN-colour IRAS source ass. with radio cont. source
IRAS17500-2405 |17 50 05.5 -24 04 48| |  (Ratag, Pottasch, 1991).
IRAS17506-2424 |17 50 39.4 -24 22 45| |PN-colour IRAS source ass. with radio cont. source
IRAS17506-2424 |17 50 39.4 -24 22 45| |  (Ratag, Pottasch, 1991).
IRAS17508-2421 |17 50 47.4 -24 22 01| |PN-colour IRAS source ass. with radio cont. source
IRAS17508-2421 |17 50 47.4 -24 22 01| |  (Ratag, Pottasch, 1991).
IRAS17510-2211 |17 51 03.7 -22 10 45| |PN-colour IRAS source ass. with radio cont. source
IRAS17510-2211 |17 51 03.7 -22 10 45| |  (Ratag, Pottasch, 1991).
IRAS17516-2525 |17 51 37.8 -25 25 58| |Either a young stellar object or a post-AGB (FC,
IRAS17516-2525 |17 51 37.8 -25 25 58| |  van der Veen etal.,1989b).
IRAS17524-2321 |17 52 25.0 -23 22 40| |PN-colour IRAS source ass. with radio cont. source
IRAS17524-2321 |17 52 25.0 -23 22 40| |  (Ratag, Pottasch, 1991).
IRAS17526-2509 |17 52 38.7 -25 10 00| |PN-colour IRAS source ass. with radio cont. source
IRAS17526-2509 |17 52 38.7 -25 10 00| |  (Ratag, Pottasch, 1991).
IRAS17532-2252 |17 53 13.5 -22 52 38| |PN-colour IRAS source ass. with radio cont. source
IRAS17532-2252 |17 53 13.5 -22 52 38| |  (Ratag, Pottasch, 1991).
IRAS17534+2603 |17 53 24.0 +26 03 24| |SAO 85545=BD+26 3120=HD 163506. 89 Her. RAFGL 2028.
IRAS17534+2603 |17 53 24.0 +26 03 24| |  F2Ibe star with far-IR excess (Parthasarathy,
IRAS17534+2603 |17 53 24.0 +26 03 24| |  Pottasch, 1986). Possible PPN (Likkel etal.,1987).
IRAS17534+2603 |17 53 24.0 +26 03 24| |  PPN cand. (Volk, Kwok, 1989, Table 1). F super-
IRAS17534+2603 |17 53 24.0 +26 03 24| |  giant as PPN cand. (Tamura etal.,1993).
IRAS17550-2741 |17 55 01.4 -27 41 52| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS17550-2741 |17 55 01.4 -27 41 52| |  1988, No.32).
IRAS17552-1841 |17 55 17.9 -18 41 17| |PN-colour IRAS source ass. with radio cont. source
IRAS17552-1841 |17 55 17.9 -18 41 17| |  (Ratag, Pottasch, 1991).
IRAS17568-2002 |17 56 50.1 -20 02 06| |PN-colour IRAS source ass. with radio cont. source
IRAS17568-2002 |17 56 50.1 -20 02 06| |  (Ratag, Pottasch, 1991).
IRAS17570-1855 |17 57 00.7 -18 55 36| |PN-colour IRAS source ass. with radio cont. source
IRAS17570-1855 |17 57 00.7 -18 55 36| |  (Ratag, Pottasch, 1991).
OH 5.89-0.39   |17 57 26.7 -24 03 56| |Young PN or peculiar HII (Zijlstra, Pottasch, 1988).
IRAS17579-3121 |17 57 59.7 -31 22 01| |PN-colour IRAS source ass. with radio cont. source
IRAS17579-3121 |17 57 59.7 -31 22 01| |  (Ratag etal.,1990, No.44).
IRAS17580-3111 |17 58 07.0 -31 11 49| |PN-colour IRAS source ass. with radio cont. source
IRAS17580-3111 |17 58 07.0 -31 11 49| |  (Ratag etal.,1990, No.45). See Hu etal.(1993a),
IRAS17580-3111 |17 58 07.0 -31 11 49| |  No.37 - coordinates different. OH 1612 MHz
IRAS17580-3111 |17 58 07.0 -31 11 49| |  detected (Hu etal.,1994).
IRAS17582-2332 |17 58 16.4 -23 33 13| |PN-colour IRAS source ass. with radio cont. source
IRAS17582-2332 |17 58 16.4 -23 33 13| |  (Ratag, Pottasch, 1991).
IRAS17588-2340 |17 58 51.4 -23 40 23| |PN-colour IRAS source ass. with radio cont. source
IRAS17588-2340 |17 58 51.4 -23 40 23| |  (Ratag, Pottasch, 1991).
IRAS17593-2345 |17 59 21.6 -23 45 34| |PN-colour IRAS source ass. with radio cont. source
IRAS17593-2345 |17 59 21.6 -23 45 34| |  (Ratag, Pottasch, 1991).
IRAS18014-1843 |18 01 30.4 -18 44 02| |PN-colour IRAS source ass. with radio cont. source
IRAS18014-1843 |18 01 30.4 -18 44 02| |  (Ratag, Pottasch, 1991).
IRAS18016-2743 |18 01 36.9 -27 43 25| |PPN cand. (FC, Hu etal.,1993a, No.33). OH 1612 MHz
IRAS18016-2743 |18 01 36.9 -27 43 25| |  detected (Hu etal.,1994).
IRAS18016-2037 |18 01 39.9 -20 37 42| |May be between OH/IR stars and PNe (Pottasch etal.,
IRAS18016-2037 |18 01 39.9 -20 37 42| |  1988, No.33).
IRAS18018-1543 |18 01 52.4 -15 43 48| |PN-colour IRAS source ass. with radio cont. source
IRAS18018-1543 |18 01 52.4 -15 43 48| |  (Ratag, Pottasch, 1991).
IRAS18020-2037 |18 02 05.2 -20 38 41| |PN-colour IRAS source ass. with radio cont. source
IRAS18020-2037 |18 02 05.2 -20 38 41| |  (Ratag, Pottasch, 1991).
IRAS18021-1928 |18 02 11.8 -19 28 28| |PN-colour IRAS source ass. with radio cont. source
IRAS18021-1928 |18 02 11.8 -19 28 28| |  (Ratag, Pottasch, 1991).
IRAS18025-3906 |18 02 35.0 -39 06 16| |PPN cand. (Kwok, 1993). See Hu etal.(1993a), No.40.
IRAS18025-3906 |18 02 35.0 -39 06 16| |  OH 1612 MHz detected (Hu etal.,1994).
IRAS18038-1830 |18 03 51.5 -18 30 02| |PN-colour IRAS source ass. with radio cont. source
IRAS18038-1830 |18 03 51.5 -18 30 02| |  (Ratag, Pottasch, 1991).
IRAS18052-1952 |18 05 13.8 -19 52 26| |PN-colour IRAS source ass. with radio cont. source
IRAS18052-1952 |18 05 13.8 -19 52 26| |  (Ratag, Pottasch, 1991).
IRAS18058-1626 |18 05 49.3 -16 26 28| |PN-colour IRAS source ass. with radio cont. source
IRAS18058-1626 |18 05 49.3 -16 26 28| |  (Ratag, Pottasch, 1991).
IRAS18061-1907 |18 06 07.7 -19 07 48| |PN-colour IRAS source ass. with radio cont. source
IRAS18061-1907 |18 06 07.7 -19 07 48| |  (Ratag, Pottasch, 1991).
IRAS18063-1943 |18 06 19.0 -19 43 17| |PN-colour IRAS source ass. with radio cont. source
IRAS18063-1943 |18 06 19.0 -19 43 17| |  (Ratag, Pottasch, 1991).
IRAS18063-2010 |18 06 21.8 -20 10 55| |PN-colour IRAS source ass. with radio cont. source
IRAS18063-2010 |18 06 21.8 -20 10 55| |  (Ratag, Pottasch, 1991).
IRAS18066-2034 |18 06 41.7 -20 34 57| |PN-colour IRAS source ass. with radio cont. source
IRAS18066-2034 |18 06 41.7 -20 34 57| |  (Ratag, Pottasch, 1991).
IRAS18072-1925 |18 07 09.0 -19 25 08| |PN-colour IRAS source ass. with radio cont. source
IRAS18072-1925 |18 07 09.0 -19 25 08| |  (Ratag, Pottasch, 1991).
IRAS18071-1727 |18 07 11.8 -17 27 28| |OH 12.8+0.9. Possibly in transition from AGB to PN
IRAS18071-1727 |18 07 11.8 -17 27 28| |  (van der Veen etal.,1989a).
IRAS18073-1839 |18 07 23.4 -18 39 49| |PN-colour IRAS source ass. with radio cont. source
IRAS18073-1839 |18 07 23.4 -18 39 49| |  (Ratag, Pottasch, 1991).
OH 11.5+0.1    |18 07 42.0 -18 53 38| |IRAS 18076-1853. "Non-variable" OH/IR star (Habing
OH 11.5+0.1    |18 07 42.0 -18 53 38| |  etal.,1987).
IRAS18084-1737 |18 08 28.1 -17 37 45| |PN-colour IRAS source ass. with radio cont. source
IRAS18084-1737 |18 08 28.1 -17 37 45| |  (Ratag, Pottasch, 1991).
IRAS18092-2146 |18 09 15.3 -21 45 56| |PN-colour IRAS source ass. with radio cont. source
IRAS18092-2146 |18 09 15.3 -21 45 56| |  (Ratag, Pottasch, 1991).
IRAS18095+2704 |18 09 30.9 +27 04 28| |High-latitude F supergiant, PPN (Hrivnak etal.,1987).
IRAS18095+2704 |18 09 30.9 +27 04 28| |  PPN (Hrivnak etal.,1999). OH 53.8+20.2; reflection
IRAS18095+2704 |18 09 30.9 +27 04 28| |  nebulosity of PPN cand. (Ueta etal.,1998).
IRAS18096-1844 |18 09 41.6 -18 44 28| |PN-colour IRAS source ass. with radio cont. source
IRAS18096-1844 |18 09 41.6 -18 44 28| |  (Ratag, Pottasch, 1991).
IRAS18100-1915 |18 10 05.0 -19 15 19| |PN-colour IRAS source ass. with radio cont. source
IRAS18100-1915 |18 10 05.0 -19 15 19| |  (Ratag, Pottasch, 1991).
IRAS18105-1935 |18 10 34.7 -19 35 56| |PPN cand. (FC, Hu etal.,1993a, No.25). OH 1612 MHz
IRAS18105-1935 |18 10 34.7 -19 35 56| |  detected (Hu etal.,1994).
IRAS18113-2503 |18 11 21.3 -25 03 52| |PPN candidate (FC, Hu etal.,1993a, No.29).
IRAS18135-1456 |18 13 32.7 -14 56 18| |Possibly in transition from AGB to PN (van der Veen
IRAS18135-1456 |18 13 32.7 -14 56 18| |  etal.,1989a). OH/IR 15.7+0.8 (Lewis, te Lintel
IRAS18135-1456 |18 13 32.7 -14 56 18| |  Hekkert, 1991).
IRAS18152-1609 |18 15 12.9 -16 09 58| |PN-colour IRAS source ass. with radio cont. source
IRAS18152-1609 |18 15 12.9 -16 09 58| |  (Ratag, Pottasch, 1991).
OH 18.5+1.4    |18 16 47.4 -12 09 27| |IRAS 18167-1209. "Non-variable" OH/IR star (Habing
OH 18.5+1.4    |18 16 47.4 -12 09 27| |  etal.,1987).
IRAS18184-1623 |18 18 25.5 -16 23 56| |HD 168625. V 4030 Sgr. Hen 1681. IR colours similar
IRAS18184-1623 |18 18 25.5 -16 23 56| |  to those observed in PNe (Parthasarathy, 1989).
IRAS18184-1623 |18 18 25.5 -16 23 56| |  PPN cand. (Meixner etal.,1999).
IRAS18184-1302 |18 18 26.7 -13 02 54| |MWC 922. PPN candidate (Meixner etal.,1999).
IRAS18213-2948 |18 21 18.0 -29 48 28| |Possibly in transition from AGB to PN (van der Veen
IRAS18213-2948 |18 21 18.0 -29 48 28| |  etal.,1989a).
IRAS18266-1239 |18 26 40.5 -12 39 56| |Possibly in transition from AGB to PN (van der Veen
IRAS18266-1239 |18 26 40.5 -12 39 56| |  etal.,1989a).
OH/IR 17.7-2.0 |18 27 39.7 -14 31 02| |IRAS 18276-1431. RAFGL 5497. Poss. PPN (Bujarrabal
OH/IR 17.7-2.0 |18 27 39.7 -14 31 02| |  etal.,1988). Between AGB and PN (FC, Le Bertre
OH/IR 17.7-2.0 |18 27 39.7 -14 31 02| |  etal.,1989). See Hu etal.(1993a), No.22.
OH/IR 17.7-2.0 |18 27 39.7 -14 31 02| |  OH 1612 MHz and CO detected (Hu etal.,1994).
IRAS18281+2149 |18 28 08.8 +21 49 50| |AC Her. HD 170756. SAO 86134. SiO maser in PPNe
IRAS18281+2149 |18 28 08.8 +21 49 50| |  (Nyman etal.,1998).
IRAS18327-0715 |18 32 47.0 -07 15 40| |Possibly in transition from AGB to PN (van der Veen
IRAS18327-0715 |18 32 47.0 -07 15 40| |  etal.,1989a).
OH 26.5+0.6    |18 34 52.5 -05 26 37| |RAFGL 2205. IRAS 18348-0526.OH/IR star (Baud, 1981).
OH 26.5+0.6    |18 34 52.5 -05 26 37| |  Possible PPN (Bujarrabal etal.,1988).
IRAS18351-2345 |18 35 07.6 -23 45 55| |SAO 187072. Colour-selected PPN candidate (Volk,
IRAS18351-2345 |18 35 07.6 -23 45 55| |  Kwok, 1989, Table 3).
OH 25.1-0.3    |18 35 33.4 -07 12 34| |IRAS 18355-0712. "Non-variable" OH/IR star (Habing
OH 25.1-0.3    |18 35 33.4 -07 12 34| |  etal.,1987).
IRAS18384-2800 |18 38 26.4 -28 00 01| |SAO 187137=HD 171894. Colour-selected PPN cand.
IRAS18384-2800 |18 38 26.4 -28 00 01| |  (Volk, Kwok, 1989, Table 3).
IRAS18450-0148 |18 45 05.2 -01 48 18| |W 43A. SiO maser in PPNe (Nyman etal.,1998).
IRAS18491-0207 |18 49 10.7 -02 07 48| |SiO maser in PPNe (Nyman etal.,1998).
IRAS18536+0753 |18 53 40.6 +07 53 22| |Possibly in transition from AGB to PN (van der Veen
IRAS18536+0753 |18 53 40.6 +07 53 22| |  etal.,1989a).
No.19-WSRT 2   |18 53 55.8 +05 49 30| |IRAS 18539+0549. IRAS-selected PN candidate; radio
No.19-WSRT 2   |18 53 55.8 +05 49 30| |  cont. data in WSRT 2 (Van de Steene, Pottasch,
No.19-WSRT 2   |18 53 55.8 +05 49 30| |  1995). FC, SECGPN (S1): VSP 4-19.
OH 37.1-0.8    |18 59 36.3 +03 15 52| |IRAS 18596+0315. OH/IR (Lewis, te Lintel Hekkert,
OH 37.1-0.8    |18 59 36.3 +03 15 52| |  1991).
IRAS19016-2330 |19 01 41.9 -23 30 45| |Possibly in transition from AGB to PN (van der Veen
IRAS19016-2330 |19 01 41.9 -23 30 45| |  etal.,1989a).
No.25-WSRT 2   |19 03 31.7 +08 01 21| |IRAS 19035+0801. Radio cont. data in WSRT 2 (Van de
No.25-WSRT 2   |19 03 31.7 +08 01 21| |  Steene, Pottasch, 1995). FC, SECGPN (S1): VSP 4-25.
No.26-WSRT 2   |19 04 10.4 +10 38 41| |IRAS 19041+1038. Radio cont. data in WSRT 2 (Van de
No.26-WSRT 2   |19 04 10.4 +10 38 41| |  Steene, Pottasch, 1995). FC, SECGPN (S1): VSP 4-26.
IRAS19067+0811 |19 06 43.7 +08 11 41| |OH 42.3-0.1. Possibly in transition from AGB to PN
IRAS19067+0811 |19 06 43.7 +08 11 41| |  (van der Veen etal.,1989a).
IRAS19075+0921 |19 07 34.0 +09 21 56| |AFGL 2333. PPN candidate (Meixner etal.,1999).
IRAS19114+0002 |19 11 24.9 +00 02 19| |SAO 124414=BD-0 3679=HD 179821. AFGL 2343. Possible
IRAS19114+0002 |19 11 24.9 +00 02 19| |  pre-PN cand. (Likkel etal.,1987). G5Ia star with
IRAS19114+0002 |19 11 24.9 +00 02 19| |  far-IR excess and colours similar to PNe (Pottasch,
IRAS19114+0002 |19 11 24.9 +00 02 19| |  Parthasarathy, 1988). Possibly in transition from
IRAS19114+0002 |19 11 24.9 +00 02 19| |  AGB to PNe (van der Veen etal.,1989a). PPN cand.
IRAS19114+0002 |19 11 24.9 +00 02 19| |  (Hrivnak etal.,1989). Colour-selected PPN cand.
IRAS19114+0002 |19 11 24.9 +00 02 19| |  (Volk, Kwok, 1989, Table 1,3). F supergiant as PPN
IRAS19114+0002 |19 11 24.9 +00 02 19| |  cand. (Tamura etal.,1993) See Arkhipova etal.
IRAS19114+0002 |19 11 24.9 +00 02 19| |  (1993), Hawkins etal.(1994), Reddy, Hrivnak (1999).
IRAS19114+0002 |19 11 24.9 +00 02 19| |  Reflection neb. of PPN cand. (Ueta etal.,1998).
IRAS19134+2131 |19 13 26.6 +21 31 13| |PPN (Nyman etal.,1998).
No.32-WSRT 1   |19 17 36.4 +12 52 01| |IRAS 19176+1251. IRAS-selected PN candidate; radio
No.32-WSRT 1   |19 17 36.4 +12 52 01| |  cont. data in WSRT 1 (Van de Steene, Pottasch,
No.32-WSRT 1   |19 17 36.4 +12 52 01| |  1995). FC, SECGPN (S1): VSP 2-31.
IRAS19192+0922 |19 19 13.2 +09 22 12| |RAFGL 2374. OH 44.8-2.3. PPN candidate (Meixner
IRAS19192+0922 |19 19 13.2 +09 22 12| |  etal.,1999).
IRAS19200+1536 |19 20 01.5 +15 36 00| |Probably late AGB star (FC, Hrivnak etal.,1985).
IRAS19244+1115 |19 24 26.3 +11 15 09| |V 1302 Aql. AFGL 2390. IRC +10420. PPN candidate
IRAS19244+1115 |19 24 26.3 +11 15 09| |  (Bujarrabal etal.,1988; Hrivnak etal.,1989).
OH 51.8-0.2    |19 25 26.0 +16 31 14| |IRAS 19254+1631. "Non-variable" OH/IR star (Habing
OH 51.8-0.2    |19 25 26.0 +16 31 14| |  etal.,1987: OH 53.8-0.2).
IRAS19288+2923 |19 28 51.4 +29 23 34| |Probably late AGB star (FC, Hrivnak etal.,1985).
IRAS19296+2227 |19 29 37.3 +22 27 16| |Water maser near PPN cand. (Marvel, Boboltz, 1998).
M 1-92         |19 34 19.2 +29 26 08| |Known as Minkowski's Footprint. VES 20 (FC, Coyne
M 1-92         |19 34 19.2 +29 26 08| |  etal.,1974). IRAS 19343+2926. Bipolar morphology,
M 1-92         |19 34 19.2 +29 26 08| |  nebular lobes and dust torus (Eiroa, Hodapp, 1989).
M 1-92         |19 34 19.2 +29 26 08| |  Binary system in process of forming a PN
M 1-92         |19 34 19.2 +29 26 08| |  (Feibelman, Bruhweiler, 1990).
No.36-WSRT 2   |19 35 21.6 +23 02 59| |IRAS 19353+2302. Radio cont. data in WSRT 2 (Van de
No.36-WSRT 2   |19 35 21.6 +23 02 59| |  Steene, Pottasch, 1995). FC, SECGPN (S1): VSP 4-36.
IRAS19374+2359 |19 37 28.7 +23 59 27| |Probably late AGB star (FC, Hrivnak etal.,1985).
IRAS19374+2359 |19 37 28.7 +23 59 27| |  PPN (Hrivnak etal.,1999). Reflection nebulosity
IRAS19374+2359 |19 37 28.7 +23 59 27| |  of PPN cand. (Ueta etal.,1998).
IRAS19386+0155 |19 38 36.5 +01 55 31| |Possibly in transition from AGB to PNe (van der Veen
IRAS19386+0155 |19 38 36.5 +01 55 31| |  etal.,1989a); A-F supergiant with large IR excess
IRAS19386+0155 |19 38 36.5 +01 55 31| |  (Arkhipova etal.,1993).
IRAS19386+1513 |19 38 39.0 +15 13 16| |Probably late AGB star (FC, Hrivnak etal.,1985).
IRAS19386+1513 |19 38 39.0 +15 13 16| |  PPN (Hrivnak etal.,1999).
HM Sge         |19 39 41.4 +16 37 33| |May be a PN in some early stage of formation
HM Sge         |19 39 41.4 +16 37 33| |  (Arkhipova, Esipov, 1976). May evolve to the
HM Sge         |19 39 41.4 +16 37 33| |  phase of a compact PN (Ciatti etal.,1977).
HM Sge         |19 39 41.4 +16 37 33| |  S1: Appendix to Table 1.
IRAS19454+2920 |19 45 24.2 +29 20 43| |Probably late AGB star (FC, Hrivnak etal.,1985).
IRAS19475+3119 |19 47 31.9 +31 19 38| |HD 331319. Possible pre-PN candidate (Likkel etal.,
IRAS19475+3119 |19 47 31.9 +31 19 38| |  1987); PPN candidate (Kwok, 1993); PPN (Hrivnak
IRAS19475+3119 |19 47 31.9 +31 19 38| |  etal.,1999).
IRAS19477+2401 |19 47 47.3 +24 01 13| |Probably late AGB star (FC, Hrivnak etal.,1985);
IRAS19477+2401 |19 47 47.3 +24 01 13| |  PPN (Hrivnak etal.,1999).
IRAS19480+2504 |19 48 02.1 +25 04 16| |PPN candidate (Kwok, 1993).
IRAS19493+2905 |19 49 21.6 +29 05 18| |Colour-selected PPN candidate (Volk, Kwok, 1989,
IRAS19493+2905 |19 49 21.6 +29 05 18| |  Table 4).
IRAS19500-1709 |19 50 00.7 -17 09 38| |SAO 163075=HD 187885; F8(I) star with far-IR excess
IRAS19500-1709 |19 50 00.7 -17 09 38| |  and colours similar to PNe (Pottasch, Parthasarathy,
IRAS19500-1709 |19 50 00.7 -17 09 38| |  1988). Possible PPN (Likkel etal.,1987). Possibly
IRAS19500-1709 |19 50 00.7 -17 09 38| |  in trans. from AGB to PN (van der Veen etal.,1989a).
IRAS19500-1709 |19 50 00.7 -17 09 38| |  Colour-selected PPN cand. (Volk, Kwok, 1989,
IRAS19500-1709 |19 50 00.7 -17 09 38| |  Table 1,3,4). PPN candidate (Hrivnak etal.,1989).
IRAS19500-1709 |19 50 00.7 -17 09 38| |  F supergiant as PPN candidate (Tamura etal.,1993).
IRAS19520+2759 |19 52 03.0 +27 59 43| |Probably late AGB star (FC, Hrivnak etal.,1985).
IRAS19548+3035 |19 54 49.2 +30 35 54| |RAFGL 2477. Probably late AGB star (FC, Hrivnak
IRAS19548+3035 |19 54 49.2 +30 35 54| |  etal.,1985).
IRAS19558+3333 |19 55 53.3 +33 33 11| |Probably late AGB star (FC, Hrivnak etal.,1985).
IRAS20000+3239 |20 00 02.8 +32 39 07| |PPN cand. (Kwok, 1993). PPN (Hrivnak etal.,1999).
IRAS20004+2955 |20 00 25.9 +29 55 53| |V 1027 Cyg. Colour-selected PPN cand. (Volk, Kwok,
IRAS20004+2955 |20 00 25.9 +29 55 53| |  1989, Table 3,4); PPN cand. (Hrivnak etal.,1989);
IRAS20004+2955 |20 00 25.9 +29 55 53| |  potential PPN (Arkhipova etal.,1992).
IRAS20028+3910 |20 02 48.0 +39 10 03| |IR colours similar to that observed in PNe (Partha-
IRAS20028+3910 |20 02 48.0 +39 10 03| |  sarathy, 1989). PPN (Hrivnak etal.,1999). Reflec.
IRAS20028+3910 |20 02 48.0 +39 10 03| |  nebulosity of PPN cand. (Ueta etal.,1998).
IRAS20043+2653 |20 04 18.2 +26 53 30| |Stellar PPN cand. (Ueta etal.,1998). PPN candidate
IRAS20043+2653 |20 04 18.2 +26 53 30| |  (Meixner etal.,1999).
IRAS20056+1834 |20 05 40.2 +18 34 10| |QY Sge. Intrinsically polarized object in the trans.
IRAS20056+1834 |20 05 40.2 +18 34 10| |  from post-AGB to PN stage (Trammell etal.,1994).
IRAS20077-0625 |20 07 47.4 -06 25 11| |V 1300 Aql. RAFGL 2514. IRC -10529. PPN candidate
IRAS20077-0625 |20 07 47.4 -06 25 11| |  (Meixner etal.,1999).
IRAS20103+3053 |20 10 22.5 +30 53 53| |Probably late AGB star (FC, Hrivnak etal.,1985).
IRAS20136+1309 |20 13 39.4 +13 09 39| |PPN (Su etal.,1999).
HBV 475        |20 49 02.6 +35 23 37| |V 1329 Cyg. May be an early stage of a PN (Crampton
HBV 475        |20 49 02.6 +35 23 37| |  etal.,1970). Symbiotic var. (Stienon etal.,1974).
HBV 475        |20 49 02.6 +35 23 37| |  S1: Appendix to Table 1.
IRAS20572+4919 |20 57 17.5 +49 19 29| |VES 351. Potential PPN (Arkhipova, Ikonnikova, 1994).
CRL 2688       |21 00 19.9 +36 29 45| |Known as Egg Nebula. May be a PPN (Lo, Bechis, 1976).
CRL 2688       |21 00 19.9 +36 29 45| |  Post-carbon-star object and prob. PN progenitor
CRL 2688       |21 00 19.9 +36 29 45| |  (Zuckerman etal.,1976). See Sahai etal.(1998), F.
CRL 2688       |21 00 19.9 +36 29 45| |  S1: Appendix to Table 1.
IRAS21027+5309 |21 02 43.3 +53 09 04| |V 1899 Cyg. Intrinsically polarized object in the
IRAS21027+5309 |21 02 43.3 +53 09 04| |  transition from post-AGB to PN stage (Trammell
IRAS21027+5309 |21 02 43.3 +53 09 04| |  etal.,1994).
IRAS21153+6842 |21 15 22.8 +68 42 18| |SAO 19283. Colour-selected PPN candidate (Volk, Kwok,
IRAS21153+6842 |21 15 22.8 +68 42 18| |  1989, Table 3).
IRAS21537+6435 |21 53 44.2 +64 35 39| |PPN candidate (Volk, Kwok, 1989, Table 1).
IRAS22036+5306 |22 03 40.0 +53 06 55| |SiO maser in PPNe (Nyman etal.,1998).
IRAS22142+5206 |22 14 14.7 +52 06 26| |Stellar PPN cand. (Ueta etal.,1998). PPN candidate
IRAS22142+5206 |22 14 14.7 +52 06 26| |  (Meixner etal.,1999).
IRAS22223+4327 |22 22 22.9 +43 27 49| |DO 41288. PPN candidate (Kwok, 1993).
IRAS22272+5435 |22 27 13.4 +54 35 44| |SAO 34504=BD+54 2787=HDE 235858. V 354 Lac. K5(I)
IRAS22272+5435 |22 27 13.4 +54 35 44| |  with far-IR excess and colours similar to PNe
IRAS22272+5435 |22 27 13.4 +54 35 44| |  (Pottasch, Parthasarathy, 1988). Possibly in trans.
IRAS22272+5435 |22 27 13.4 +54 35 44| |  from AGB to PNe (van der Veen etal.,1989a). Likely
IRAS22272+5435 |22 27 13.4 +54 35 44| |  between AGB and PNe (Kwok etal.,1989). Colour-se-
IRAS22272+5435 |22 27 13.4 +54 35 44| |  lected PPN cand. (Volk, Kwok, 1989, Table 1,3,4);
IRAS22272+5435 |22 27 13.4 +54 35 44| |  see also Hrivnak, Kwok (1991), Arkhipova etal.
IRAS22272+5435 |22 27 13.4 +54 35 44| |  (1993) and Meixner etal.(1994). Reflection nebu-
IRAS22272+5435 |22 27 13.4 +54 35 44| |  losity of PPN cand. (Ueta etal.,1998).
IRAS22480+6002 |22 48 00.9 +60 02 01| |PPN candidate (Meixner etal.,1999).
IRAS22574+6609 |22 57 25.1 +66 09 42| |PPN candidate (Kwok, 1993). PPN (Hrivnak etal.,1999).
IRAS22574+6609 |22 57 25.1 +66 09 42| |  Reflection neb. of PPN cand. (Ueta etal.,1998).
IRAS23166+1655 |23 16 42.4 +16 55 10| |AFGL 3068. PPN candidate (Meixner etal.,1999).
IRAS23268+6854 |23 26 49.8 +68 54 23| |Probably late AGB star (FC, Hrivnak etal.,1985).
IRAS23304+6147 |23 30 26.7 +61 47 15| |Likely between AGB and PNe (Kwok etal.,1989).Post-AGB
IRAS23304+6147 |23 30 26.7 +61 47 15| |  stage (FC, Reddy, Parthasarathy, 1996).PPN (Hrivnak
IRAS23304+6147 |23 30 26.7 +61 47 15| |  etal.,1999).
IRAS23321+6545 |23 32 06.3 +65 45 15| |Pre-PN cand. (Likkel etal.,1987). Colour-selected PPN
IRAS23321+6545 |23 32 06.3 +65 45 15| |  candidate (Volk, Kwok, 1989, Table 4). Reflection
IRAS23321+6545 |23 32 06.3 +65 45 15| |  nebulosity of PPN cand. (Ueta etal.,1998).
IRAS23416+6130 |23 41 38.8 +61 30 43| |PZ Cas. BD+60 2613. IRC +60417. Intrinsically pola-
IRAS23416+6130 |23 41 38.8 +61 30 43| |  rized object in the transition from post-AGB to
IRAS23416+6130 |23 41 38.8 +61 30 43| |  PN stage (Trammell etal.,1994).
----------------------------------------------------------------------------------------------