Table 5
IR luminosity, H2O line luminosity and global dust temperature of the entire sample.
| Source | H2O Transition | LIR | LH2O(211–202) | LH2O(202–111) | LH2O(321–312) |
| (1012 L⊙) | (107 L⊙) | (107 L⊙) | (107 L⊙) | ||
|
|
|||||
| G09v1.97 | 211–202 , 321–312 | 22.1 ± 5.9 | 10.7 ± 1.4 | – | 15.0 ± 1.9 |
| G12v2.43 | 202–111 , 321–312 | 83.2 ± 16.6 /μ | – | 88.4 ± 10.7 /μ | 143.2 ± 11.5 /μ |
| NCv1.143 | 211–202 , 321–312 | 11.4 ± 3.1 | 9.0 ± 1.4 | – | 18.9 ± 3.3 |
| NAv1.195 | 202–111 , 321–312 | 18.0 ± 4.6 | – | 16.4 ± 3.0 | < 12.3 |
| NAv1.177 | 202–111 , 321–312 | 55.0 ± 11.0 /μ | – | 82.0 ± 12.8 /μ | 129.1 ± 10.8 /μ |
| NBv1.78 | 202–111 , 321–312 | 8.2 ± 2.2 | – | 9.4 ± 2.1 | 11.0 ± 1.5 |
|
|
|||||
| G09v1.124-W | 211–202 | 33.1 ± 3.2 | < 12.9 | – | – |
| G09v1.124-T | 211–202 | 14.5 ± 1.8 | < 6.9 | – | – |
| G09v1.40 | 211–202 | 4.2 ± 1.3 | 3.7 ± 0.9 | – | – |
| SDP11 | 202–111 | 5.7 ± 1.6 | – | 5.8 ± 1.4 | – |
| NCv1.268 | 211–202 | 8.6 ± 2.3 | 11.5 ± 1.5 | – | – |
| NAv1.56 | 211–202 | 9.7 ± 2.6 | 10.3 ± 1.2 | – | – |
|
|
|||||
| SDP81 | 202–111 | 6.1 | – | 3.3 | – |
| NAv1.144 | 211–202 | 11 | 9.7 | – | – |
| SDP9 | 211–202 | 5.2 | 7.0 | – | – |
| G12v2.30 | 202–111 | 16 | – | 13 | – |
| SDP17b | 202–111 | 16 | – | 20 | – |
| G15v2.779 | 211–202 | 21 | 26.6 | – | – |
Notes.LIR is the intrinsic total infrared luminosity (8–1000 μm) taken from B13. The intrinsic H2O luminosities are inferred from μLH2O using μ in B13. The first group of the sources are the ones with both J = 2 and J = 3 H2O lines observed, the next group are the sources with only J = 2 H2O observed, and the last group are the previous published sources in O13.
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