Table 1
Post-AGB sources observed with the 30 m IRAM telescope.
| Source | Observed coordinates | F 25 μ | F 60 μ | Luminosity | Distance | sp. type | V∗(LSR) | Comments | |
| J2000 | Jy | Jy | L ⊙ | pc | km s-1 | ||||
|
|
|||||||||
| RV Tau | 04:47:06.73 | +26:10:45.6 | 18.1 | 6.5 | 3500 | 22001 | G2-M2 | +17 | RV Tau variable |
| DY Ori | 06:06:14.91 | +13:54:19.1 | 14.9 | 4.2 | 1600 | 20001 | G0 I | –16 | RV Tau variable |
| Red Rectangle | 06:19:58.22 | –10:38:14.7 | 456.1 | 173.1 | 6000 | 7102 | B9 | 0 | interferometric CO maps |
| U Mon | 07:30:47.47 | –09:46:36.8 | 88.4 | 26.6 | 4000 | 8001 | F8-K0 I | +9 | RV Tau variable |
| AI CMi | 07:35:41.15 | +00:14:58.0 | 68.1 | 18.5 | 30003 | 15003 | G5 I | +33 | |
| HR 4049 | 10:18:07.59 | –28:59:31.2 | 9.6 | 1.8 | 2900 | 6504 | A6 I | –45 | well studied inner disk |
| 89 Her | 17:55:25.19 | +26:03:00.0 | 54.5 | 13.4 | 9200 | 10005 | F2 I | –8 | interferometric CO maps |
| IRAS 18123+0511 | 18:14:49.39 | +05:12:55.7 | 11.0 | 4.2 | 30003 | 35003 | F2 | +99 | |
| AC Her | 18:30:16.24 | +21:52:00.6 | 65.3 | 21.4 | 3500 | 11001 | F2-K4 I | –10 | previous tent. det., RV Tau variable |
| R Sct | 18:47:28.95 | –05:42:18.5 | 9.3 | 8.2 | 14000 | 10005 | G0-K0 I | +55 | previous det., pec. RV Tau variable |
| IRAS 19125+0343 | 19:15:01.18 | +03:48:42.7 | 26.5 | 7.8 | 30003 | 15003 | F2 | +84 | |
| IRAS 19157-0247 | 19:18:22.71 | –02:42:10.9 | 7.2 | 2.5 | 30003 | 29003 | F3 | +49 | |
| IRAS 20056+1834 | 20:07:54.62 | +18:42:54.5 | 18.0 | 5.4 | 30003 | 30003 | G0 | ~0 | edge-on disk |
| R Sge | 20:14:03.75 | +16:43:35.1 | 7.5 | 2.1 | 2500 | 25001 | G0-K0 I | +28 | RV Tau variable |
Notes. Observed coordinates and other relevant properties including IRAS fluxes, total luminosity and adopted distance (Sect. 2.1), stellar spectral type, and stellar velocity (derived from optical lines, except for sources previously detected in CO emission) are listed. Distance estimate:
Men’shchikov et al. (2002);
Corrected parallax (Acke et al. 2013);
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