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Table 1
CO and H2O rotational excitation.
| Source | D | Lbol | Warm CO | Hot CO | H2O | |||||||||
| (pc) | (L⊙) | Trot (K) |
|
Trot (K) |
|
Trot (K) |
|
|||||||
|
|
||||||||||||||
| AFGL 490 | 1000 | 2000 | 300(20) | 51.6(0.1) | ... | ... | 90(100) | 48.3(1.2) | ||||||
| L 1641 S3 MMS1 | 465 | 70 | 325(30) | 49.9(0.1) | ... | ... | 150(100) | 46.8(0.1) | ||||||
| NGC 2071 | 422 | 520 | 310(30) | 51.2(0.1) | 700(50) | 50.1(0.1) | 135(100) | 47.9(0.1) | ||||||
| Vela 17 | 700 | 715 | 265(25) | 50.8(0.2) | ... | ... | 90(40) | 47.8(0.5) | ||||||
| Vela 19 | 700 | 776 | 335(50) | 50.4(0.2) | ... | ... | 130(80) | 47.2(0.4) | ||||||
| NGC 7129 FIRS 2 | 1250 | 430 | 370(45) | 50.7(0.2) | 710(70) | 49.9(0.2) | 130(50) | 47.8(0.1) | ||||||
Notes. Distances and bolometric luminosities are taken from Wampfler et al. (2013) and references therein.
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