Table 1
Properties of the AGB stars.
| IRAS | Other name | l | b | Chem. | d | V exp | Ṁ | f12 | f12/f25 | Refs. |
| (pc) | (km s-1) | (10-5M⊙ yr-1) | (Jy) | |||||||
|
|
||||||||||
| 00193−4033 | AFGL 5017 | 326 | −75 | O | 360 | 17.3 | 0.10 | 312 | 2.07 | 1 |
| 01037+1219 | IRC+10011 | 128 | −50 | O | 740 | 21.6 | 2.2 | 1155 | 1.19 | 2 |
| 04575+1251 | AFGL 5134 | 188 | −18 | O | 1200 | 12.9 | 1.0 | 133 | 1.09 | 3, 4, 9 |
| 05418−3224 | 237 | −27 | C | 4300 | 10.0 | 1.1 | 63 | 2.47 | 5 | |
| 06012+0726 | AFGL 865 | 201 | −07 | C | 1470 | 16.6 | 1.8 | 320 | 1.42 | 5 |
| 06255−4928 | 258 | −24 | O | 1100 | 15.0 | 0.31 | 66 | 1.53 | 4, 9, 10 | |
| 07454−7112 | AFGL 4078 | 283 | −21 | C | 940 | 13.5 | 1.6 | 613 | 1.99 | 5 |
| 09116−2439 | AFGL 5254 | 253 | +16 | C | 940 | 12.8 | 1.3 | 737 | 1.85 | 5 |
| 09452+1330 | IRC+10216 | 221 | +45 | C | 120 | 14.7 | 1.75 | 47 500 | 2.06 | 6 |
| 09521−7508 | AFGL 4098 | 292 | −16 | C | 1300 | 12.8 | 1.1 | 345 | 1.86 | 5 |
| 10323−4611 | 280 | +10 | O | 580 | 20.4 | 1.0 | 537 | 1.46 | 4, 9 | |
| 12384−4536 | 301 | +19 | O | 1100 | 8.1 | 0.20 | 159 | 2.25 | 1 | |
| 14591−4438 | 326 | +12 | O | 600 | 15.2 | 0.25 | 304 | 1.47 | 1 | |
| 16029−3041 | AFGL 1822 | 345 | +16 | O | 1900 | 16.8 | 1.10 | 141 | 0.53 | 1 |
| 17319−6234 | OH 329.8−15.8 | 330 | −16 | O | 1200 | 17.5 | 0.84 | 252 | 0.85 | 1 |
| 18240+2326 | AFGL 2155 | 52 | +16 | C | 920 | 15.1 | 0.46 | 731 | 1.63 | 5 |
| 18467−4802 | OH 348.2−19.7 | 348 | −20 | O | 1200 | 12.3 | 0.78 | 285 | 0.83 | 1 |
| 19178−2620 | AFGL 2370 | 12 | −18 | O | 2200 | 18.0 | 1.3 | 78 | 0.81 | 1 |
| 20042−4241 | AFGL 5578 | 358 | −31 | O | 460 | 14.4 | 0.15 | 221 | 1.41 | 7, 8 |
| 20077−0625 | AFGL 2514 | 36 | −20 | O | 760 | 16.0 | 1.7 | 1255 | 1.18 | 2 |
| 23257+1038 | AFGL 3099 | 92 | −47 | C | 1610 | 10.5 | 0.85 | 190 | 1.34 | 5 |
| 23320+4316 | AFGL 3116 | 108 | −17 | C | 780 | 14.7 | 0.70 | 959 | 2.04 | 5 |
References. (1) d, V, and Ṁ from Loup et al. (1993); (2) d, V, and Ṁ from Olivier et al. (2001); (3) V from OH observations, David et al. (1993); (4) Ṁ estimated through a correlation of Ṁ with the K − [12] color, where K is from the 2MASS catalog, and [12] = −2.5 log (f12/28.3), with f12 from the IRAS point-source catalog; (5) d, V, and Ṁ from Groenewegen et al. (2002); (6) d from Ramstedt et al. (2008), Ṁ from Schöier & Olofsson (2001), Vexp from Loup et al. (1993); (7) V from Loup et al. (1993); (8) d and Ṁ from Whitelock et al. (1994); (9) d estimated assuming L = 3500 L⊙ (e.g., Jackson et al. 2002); (10) No Vexp available, 15 km s-1 adopted value.
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