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APPENDIX A to TABLE 1      Possible PRE-PLANETARY NEBULAE (1995-1999)

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Name              RA   (1950)   DEC   Remarks and references
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                 h  m  s     o  '  "
IRAS00470+6429  00 47 02.9 +64 29 16  PPN candidate (Meixner etal.,1999).
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. 
                                        (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.,
                                        1997). Reflection nebulosity of PPN cand. (Ueta
                                        etal.,1998). Carbon-rich PPN (Reddy etal.,1999).
HD 20041        03 11 57.1 +56 57 22  LSI+56 85. SAO 23903. PPN candidate (Meixner etal.,
                                        1999).
IRAS04386+5722  04 38 38.2 +57 22 11  PPN candidate (Meixner etal.,1999). Stellar PPN
                                        cand. (Ueta etal.,1998).
IRAS05089+0459  05 08 56.6 +04 59 50  PPN candidate (Meixner etal.,1999).
IRAS05238-0626  05 23 53.1 -06 26 29  BD-06 1178. Most likely post-AGB supergiant evolving
                                        towards PN (F, Reddy, Parthasarathy, 1996). 
No.6-WSRT 2     06 25 15.2 +12 48 56  IRAS 06252+1248. IRAS-selected PN candidate; radio
                                        cont. data in WSRT 2 (Van de Steene, Pottasch,
                                        1995). F, S1 to SECGPN: VSP 4-6.
IRC -20101      06 39 08.3 -22 13 47  RAFGL 4521S. Possible pre-PN (Likkel etal.,1987). 
HD 51585        06 55 37.6 +16 23 32  Evolving towards early stages of PNe (Parthasarathy,
                                        Pottasch, 1989).
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 (F, Reddy, Parthasa-
                                        rathy, 1996).
IRAS07284-0940  07 28 24.3 -09 40 15  HD 59693. U Mon. SAO 134775. PPN candidate (Meixner 
                                        etal.,1999).
OH 231.8+4.2    07 39 58.9 -14 35 44  QX Pup. IRAS 07399-1435. Known as Rotten Egg Nebula.
                                        Possible PPN (Bujarrabal etal.,1988). See Morris 
                                        etal.(1987).
IRAS07430+1115  07 43 04.2 +11 15 46  In transition between AGB and PNe (Hrivnak etal.,
                                        1997). Reflection neb. of PPN cand. (Ueta etal.,
                                        1998). Carbon-rich PPN (Reddy etal.,1999).
IRAS07536-2830  07 53 38.4 -28 30 54  HU Pup. SAO 174817. Intrinsically polarized object 
                                        in the transition from post-AGB to PN stage 
                                        (Trammell etal.,1994).
IRAS07582-4059  07 58 14.4 -40 59 07  PPN candidate (F, Hu etal.,1993, No.42).
IRAS08143-4406  08 14 23.1 -44 06 43  Most likely in post-AGB stage (F, Reddy, Parthasa-
                                        rathy, 1996).
IRAS08187-1905  08 18 42.6 -19 05 30  HD 70379. Most likely post-AGB supergiant evolving
                                        towards PN (F, Reddy, Parthasarathy, 1996).
IRAS09370-4826  09 37 03.5 -48 26 34  PPN candidate (F, Hu etal.,1993, No.47).
IRAS09371+1212  09 37 12.0 +12 12 31  Peculiar galaxy (F, Condon, Broderick, 1986). Known 
                                        as Frosty Leo Nebula. Possible pre-PN (Likkel 
                                        etal.,1987). Evolved, mass-losing red giant, 
                                        post-AGB circumstellar envelope (F, Forveille 
                                        etal.,1987). Possible PPN (Bujarrabal etal.,1988). 
                                        Pre-main-sequence young object? (Robinson etal., 
                                        1992).
IRAS10029-5553  10 02 54.6 -55 54 01  PPN candidate (F, Hu etal.,1993, No.49). IRAS-radio 
                                        PN candidate (Van de Steene, Pottasch, 1993).
IRAS10131+3049  10 13 10.7 +30 49 17  RW LMi. RAFGL 1403. IRC +30219. PPN candidate 
                                        (Meixner etal.,1999).
IRC -10236      10 14 34.5 -14 24 30  IY Hya. Intrinsically polarized object in the tran-
                                        sition from post-AGB to PN stage (Trammell etal.,
                                        1994).
IRAS10491-2059  10 49 11.3 -20 59 04  V Hya. BD-20 3283. SAO 179278. IRC -20218. Intrin-
                                        sically polarized object in the transition from 
                                        post-AGB to PN stage (Trammell etal.,1994).
IRAS11339-6004  11 33 59.9 -60 04 20  PPN candidate (F, Hu etal.,1993, No.53).
IRAS11381-6401  11 38 10.4 -64 01 49  PPN candidate (F, Hu etal.,1993, No.60).
IRAS11387-6113  11 38 47.8 -61 13 51  PPN candidate (F, Hu etal.,1993, 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 (F, Hu etal.,1993, No.61).
1200-5333       12 00 13.3 -53 33 24  IRAS-radio PN candidate (Van de Steene, Pottasch,
                                        1993).
IRAS12309-5928  12 30 55.0 -59 28 45  PPN candidate (F, Hu etal.,1993, No.51).
IRAS12323-2033  12 32 19.1 -20 33 39  RU Crv. BD-20 3674. SAO 180922. IRC -20241. Intrin-
                                        sically polarized object in the transition from 
                                        post-AGB to PN stage (Trammell etal.,1994).
IRAS12358-6323  12 35 53.2 -63 23 10  PPN cand. (F, Hu etal.,1993, No.59). OH 1612 MHz
                                        detected (Hu etal.,1994).
IRAS12359+0715  12 35 57.6 +07 15 48  R Vir. HD 109914. SAO 119509. IRC +10256. Intrin-
                                        sically polarized object in the transition from 
                                        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,
                                        1993).
ESO-172?07      12 41 54.2 -54 14 47  IRAS 12419-5414. Known as Boomerang Nebula, re-
                                        flection nebula. CO obs. of PPNe (Bujarrabal, 
                                        Bachiler, 1991).
IRAS12447+0425  12 44 45.6 +04 25 05  RU Vir. BD+04 2651a=HD 111166. IRC +00224. Intrin-
                                        sically polarized object in the transition from 
                                        post-AGB to PN stage (Trammell etal.,1994). 
IRAS13404-6059  13 40 26.8 -60 59 41  PPN candidate (F, Hu etal.,1993, No.54).
IRAS14122-5947  14 12 13.4 -59 47 19  PPN candidate (F, Hu etal.,1993, No.52).
He 3-1031       14 33 07.4 -64 35 01  IRAS 14331-6435. CPD-64 2939.Evolving towards early 
                                        stages of PNe (Parthasarathy, Pottasch, 1989).
IRAS14341-6211  14 34 10.2 -62 11 42  PPN cand. (F, Hu etal.,1993, No.57). OH 1612 MHz
                                        detected (Hu etal.,1994).
IRAS14429-4539  14 42 55.2 -45 39 31  PPN cand. (F, Hu etal.,1993, No.44). Most likely 
                                        in post-AGB stage (F, Reddy, Parthasarathy, 1996).
IRAS14527-6204  14 52 43.4 -62 04 49  PPN candidate (F, Hu etal.,1993, No.56).
1510-5754       15 10 25.2 -57 54 11  IRAS-radio PN candidate (Van de Steene, Pottasch,
                                        1993).
IRAS15255+1944  15 25 32.2 +19 44 10  WX Ser. IRC +20281. Intrinsically polarized object 
                                        in the transition from post-AGB to PN stage 
                                        (Trammell etal.,1994).
IRAS15405-4945  15 40 32.1 -49 45 54  OH 329.14+3.92. SiO maser in PPNe (Nyman etal., 
                                        1998). See te Lintel Hekkert etal.(1988). 
IRAS16029-4101  16 02 59.4 -41 01 52  PPN candidate (F, Hu etal.,1993, No.43).
IRAS16032-3537  16 03 12.2 -35 37 19  IRAS PSC PN candidate (F Carballo etal.,1992).
IRAS16086-5255  16 08 37.4 -52 55 44  PPN candidate (F, Hu etal.,1993, No.48).
IRAS16130-4620  16 13 06.3 -46 20 36  PPN candidate (F, Hu etal.,1993, No.45).
IRC +30292      16 26 00.6 +34 54 45  V 697 Her. IRAS 16260+3454. Intrinsically pola-
                                        rized object in the transition from post-AGB to 
                                        PN stage (Trammell etal.,1994). 
1633-4807       16 33 23.4 -48 07 40  IRAS-radio PN candidate (Van de Steene, Pottasch,
                                        1993).
IRAS16552-3050  16 55 16.5 -30 50 37  PPN candidate (F, Hu etal.,1993, No.35).
IRAS16559-2957  16 55 57.4 -29 57 09  PPN candidate (F, Hu etal.,1993, No.34). OH 1612 MHz
                                        detected (Hu etal.,1994).
IRAS17106-3046  17 10 38.9 -30 46 13  PPN (Hrivnak etal.,1999). PPN candidate (Meixner 
                                        etal.,1999).
IRAS17195-2710  17 19 35.9 -27 10 48  Heavily-reddened low-exc. em.-line object (F, Hu 
                                        etal.,1993a, No.31). S1 to SECGPN: GLMP 554.
IRAS17233-2602  17 23 22.6 -26 02 25  PPN candidate (F, Hu etal.,1993, No.30). OH 0.1+5.1
                                        (Hu etal.,1994).
IRAS17385-3332  17 38 34.4 -33 32 14  PPN candidate (F, Hu etal.,1993, No.39). OH 1612 MHz
                                        detected (Hu etal.,1994).
IRAS17433-1750  17 43 20.6 -17 50 36  PPN candidate (F, Hu etal.,1993, No.24). OH 1612 MHz
                                        detected (Hu etal.,1994).
IRAS17456-2037  17 45 41.5 -20 37 15  PPN candidate (F, Hu etal.,1993, No.26).
IRAS18016-2743  18 01 36.9 -27 43 25  PPN cand. (F, Hu etal.,1993, No.33). OH 1612 MHz
                                        detected (Hu etal.,1994).
IRAS18105-1935  18 10 34.7 -19 35 56  PPN cand. (F, Hu etal.,1993, No.25). OH 1612 MHz
                                        detected (Hu etal.,1994).
IRAS18113-2503  18 11 21.3 -25 03 52  PPN candidate (F, Hu etal.,1993, No.29).
IRAS18184-1302  18 18 26.7 -13 02 54  MWC 922. PPN candidate (Meixner etal.,1999).
IRAS18281+2149  18 28 08.8 +21 49 50  AC Her. HD 170756. SAO 86134. SiO maser in PPNe 
                                        (Nyman etal.,1998).
OH 26.5+0.6     18 34 52.5 -05 26 37  RAFGL 2205. IRAS 18348-0526. OH/IR star (Baud,1981). 
                                        Possible PPN (Bujarrabal etal.,1988).
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).
No.19-WSRT 2    18 53 55.8 +05 49 30  IRAS 18539+0549. IRAS-selected PN candidate; radio
                                        cont. data in WSRT 2 (Van de Steene, Pottasch,
                                        1995). F, S1 to SECGPN: VSP 4-19.
No.25-WSRT 2    19 03 31.7 +08 01 21  IRAS 19035+0801. Radio cont. data in WSRT 2 (Van de 
                                        Steene, Pottasch, 1995). F, S1 to SECGPN: 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 
                                        Steene, Pottasch, 1995). F, S1 to SECGPN: VSP 4-26.
IRAS19075+0921  19 07 34.0 +09 21 56  AFGL 2333. PPN candidate (Meixner etal.,1999).
IRAS19134+2131  19 13 26.6 +21 31 13  PPN (Nyman etal.,1998).
No.31-WSRT 1    19 17 36.4 +12 52 01  IRAS 19176+1251. IRAS-selected PN candidate; radio
                                        cont. data in WSRT 1 (Van de Steene, Pottasch,
                                        1995). F, S1 to SECGPN: VSP 2-31.
IRAS19192+0922  19 19 13.2 +09 22 12  RAFGL 2374. OH 44.8-2.3. PPN candidate (Meixner 
                                        etal.,1999).
IRAS19296+2227  19 29 37.3 +22 27 16  Water maser near PPN cand. (Marvel, Boboltz, 1998).
No.36-WSRT 2    19 35 21.6 +23 02 59  IRAS 19353+2302. Radio cont. data in WSRT 2 (Van de 
                                        Steene, Pottasch, 1995). F, S1 to SECGPN: VSP 4-36.
IRAS20043+2653  20 04 18.2 +26 53 30  PPN candidate (Meixner etal.,1999). Stellar PPN
                                        cand. (Ueta etal.,1998).
IRAS20056+1834  20 05 40.2 +18 34 10  QY Sge. Intrinsically polarized object in the 
                                        transition 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 
                                        (Meixner etal.,1999).
IRAS20136+1309  20 13 39.4 +13 09 39  PPN (Su etal.,1999).
IRAS21027+5309  21 02 43.3 +53 09 04  V 1899 Cyg. Intrinsically polarized object in the 
                                        transition from post-AGB to PN stage (Trammell 
                                        etal.,1994).
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  PPN candidate (Meixner etal.,1999). Stellar PPN
                                        cand. (Ueta etal.,1998).
IRAS22480+6002  22 48 00.9 +60 02 01  PPN candidate (Meixner etal.,1999).
IRAS23166+1655  23 16 42.4 +16 55 10  AFGL 3068. PPN candidate (Meixner etal.,1999).
IRAS23416+6130  23 41 38.8 +61 30 43  PZ Cas. BD+60 2613. IRC +60417. Intrinsically pola-
                                        rized object in the transition from post-AGB to 
                                        PN stage (Trammell etal.,1994).
________________________________________________________________________________________


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Nächste Seite: APPENDIX B to TABLE 1 Aufwärts: text Vorherige Seite: TABLE 1

Lubos Kohoutek
2001-03-15