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| Query : 1995A&A...299...69O |
1995A&A...299...69O - Astronomy and Astrophysics, volume 29969-78 (1995/7-1)
Near-infrared spectroscopy of post-AGB stars.
OUDMAIJER R.D., WATERS L.B.F.M., VAN DER VEEN W.E.C.J. and GEBALLE T.R.
Abstract (from CDS):
The results of a medium resolution near-infrared spectral survey of 18 post-AGB candidate stars are presented. Most of the stars have near-infrared hydrogen lines in absorption, which is normal for their spectral types. Three stars, HD 101584, HD 179821 and HD 170756 have the CO first overtone bands in emission; in two of these the emission is variable. It is suggested that the CO emission is the result of post-AGB mass loss. HD 52961 shows the rarely occurring 3.5µm emission feature and is only the fourth object in which this feature has been detected.
Abstract Copyright: ∼
Journal keyword(s): stars: circumstellar matter - stars: evolution - stars: mass loss - stars: AGB and post-AGB
Simbad objects: 39
| Number of rows : 39 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | V* RV Tau | RV* | 04 47 06.7239850584 | +26 10 45.532913268 | 11.00 | 9.80 | K3Ibe | 297 | 1 | |||
| 2 | * pi.03 Ori | PM* | 04 49 50.4112051485 | +06 57 40.600622266 | 3.620 | 3.630 | 3.190 | 2.77 | 2.51 | F6V | 601 | 0 |
| 3 | * kap Aur | PM* | 06 15 22.6883791803 | +29 29 53.075320396 | 6.17 | 5.36 | 4.35 | 3.55 | 3.01 | G8.5IIIb | 218 | 0 |
| 4 | HD 44179 | pA* | 06 19 58.2185496 | -10 38 14.706068 | 9.51 | 9.33 | 9.02 | B9Ib/II | 800 | 0 | ||
| 5 | * gam Gem | SB* | 06 37 42.71050 | +16 23 57.4095 | 1.98 | 1.92 | 1.92 | 1.86 | 1.87 | A1.5IV+ | 525 | 1 |
| 6 | V* PS Gem | pA* | 07 03 39.6305052432 | +10 46 13.068774048 | 7.76 | 7.37 | A0 | 130 | 0 | |||
| 7 | HD 53300 | pA? | 07 04 19.4780299008 | -05 18 19.551600720 | 8.73 | 8.37 | 8.06 | A2II | 24 | 0 | ||
| 8 | HD 56126 | pA* | 07 16 10.2590823192 | +09 59 47.954735376 | 9.20 | 8.32 | F0/5Ia | 330 | 0 | |||
| 9 | V* U Mon | pA* | 07 30 47.4711645432 | -09 46 36.757477488 | 8.22 | 7.00 | 5.82 | G8/K0Ib/II | 215 | 0 | ||
| 10 | * 18 Pup | PM* | 08 10 39.8256078504 | -13 47 57.141934620 | 6.03 | 5.54 | F6.5V | 166 | 0 | |||
| 11 | HD 89353 | pA* | 10 18 07.5899342712 | -28 59 31.195183524 | 5.76 | 5.53 | B9.5Ib/II | 315 | 0 | |||
| 12 | HD 97651 | * | 11 13 39.3932239752 | -53 13 54.533999460 | 7.045 | 5.740 | K2III | 21 | 0 | |||
| 13 | * A Cen | Be* | 11 34 45.6563651706 | -54 15 50.735175236 | 4.33 | 4.533 | 4.607 | B9V | 81 | 0 | ||
| 14 | HD 101584 | pA* | 11 40 58.8051522552 | -55 34 25.814696232 | 7.80 | 7.40 | 7.01 | B8/9I/IIe | 156 | 0 | ||
| 15 | V* V918 Cen | LP* | 11 47 19.1412363000 | -57 41 47.402548440 | 7.055 | 5.407 | K5III | 53 | 0 | |||
| 16 | HD 139129 | * | 15 38 49.4705005656 | -52 22 21.709310952 | 5.421 | 5.423 | A0V | 64 | 0 | |||
| 17 | IRAS 15452-5459 | pA* | 15 49 11.3344710672 | -55 08 51.846940176 | O-rich | 34 | 0 | |||||
| 18 | IRAS 16115-5044 | s*b | 16 15 17.9553965760 | -50 52 19.841361852 | ~ | 26 | 0 | |||||
| 19 | * eps Nor | SB* | 16 27 11.0416112400 | -47 33 17.257138078 | 4.439 | 4.521 | B2V | 71 | 0 | |||
| 20 | IRAS 17516-2525 | pA* | 17 54 43.3459663104 | -25 26 28.127732028 | O-B? | 39 | 1 | |||||
| 21 | * gam02 Sgr | PM* | 18 05 48.4880988 | -30 25 26.723458 | 4.77 | 4.00 | 2.99 | 2.26 | 1.75 | K0+III | 158 | 0 |
| 22 | OH 015.7+00.8 | OH* | 18 16 25.77744 | -14 55 13.7388 | O-rich | 77 | 0 | |||||
| 23 | V* AC Her | pA* | 18 30 16.2373118976 | +21 52 00.599340000 | 8.00 | 7.79 | 7.01 | F4Ibp | 359 | 0 | ||
| 24 | HD 175156 | * | 18 54 43.1136473552 | -15 36 10.932683925 | 5.208 | 5.086 | B3II | 136 | 0 | |||
| 25 | * g Aql | ** | 19 02 54.5010526943 | -03 41 56.288077922 | 5.39 | 5.40 | B9IV | 55 | 0 | |||
| 26 | HD 179821 | pA* | 19 13 58.6082398776 | +00 07 31.935181836 | 10.81 | 9.694 | 8.19 | G4_0-Ia | 247 | 0 | ||
| 27 | HD 186438 | pA* | 19 42 52.9222053048 | +37 40 41.459108880 | 8.73 | 8.32 | 7.91 | F3Ib | 31 | 0 | ||
| 28 | * f Sgr | PM* | 19 46 21.7395133902 | -19 45 40.012615240 | 5.930 | 4.873 | K0+III | 73 | 0 | |||
| 29 | HD 187885 | pA* | 19 52 52.7033593752 | -17 01 50.289441096 | 9.25 | 8.68 | 8.32 | F2/6Ia | 185 | 0 | ||
| 30 | V* V1401 Aql | pA* | 20 05 05.4136151160 | -11 35 57.894584100 | 6.88 | 6.39 | F2II | 119 | 0 | |||
| 31 | V* R Sge | pA* | 20 14 03.7432133928 | +16 43 35.030552844 | 10.19 | 9.20 | G8Ib | 86 | 0 | |||
| 32 | * gam Cyg | V* | 20 22 13.7018357 | +40 15 24.044963 | 3.44 | 2.90 | 2.23 | 1.74 | 1.40 | F8Ib | 607 | 0 |
| 33 | * 42 Cyg | pA* | 20 29 20.3901455688 | +36 27 17.017726104 | 6.291 | 5.899 | A2Iab-Ib | 92 | 0 | |||
| 34 | * 70 Aql | * | 20 36 43.6331948352 | -02 32 59.836714368 | 6.475 | 4.880 | K4+IIIBa1 | 83 | 0 | |||
| 35 | HD 235858 | pA* | 22 29 10.3748806056 | +54 51 06.344572284 | 11.40 | 9.52 | 8.47 | 7.34 | G5Ia | 264 | 0 | |
| 36 | * sig Aqr | * | 22 30 38.8214037672 | -10 40 40.505006280 | 4.59 | 4.73 | 4.81 | 4.81 | 4.85 | A0IVs | 125 | 0 |
| 37 | HD 213985 | pA* | 22 35 27.5260668720 | -17 15 26.894587392 | 9.31 | 9.08 | 8.90 | A0III | 118 | 0 | ||
| 38 | * g Aqr | V* | 22 43 35.2332465969 | -18 49 49.350293114 | 6.06 | 4.69 | K3III | 60 | 0 | |||
| 39 | BD+39 4926 | pA* | 22 46 11.2272974832 | +40 06 26.309865960 | 9.621 | 9.357 | 9.374 | A0IIp | 130 | 0 |
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