Table 7
H2O rotational temperatures and total number of molecules.
| YSO | T a |
a
|
| [K] | [1045] | |
|
|
||
| IRS7A+SMM 1C | 197 ± 4 | 10.1 ± 0.3 |
| IRS7B | 174 ± 4 | 2.3 ± 0.1 |
| R CrA | 235 ± 9 | 1.3 ± 0.1 |
| IRS5A | 185 ± 5 | 1.2 ± 0.1 |
| IRS5N | 195 ± 20 | 0.5 ± 0.1 |
|
|
||
| Res SW-l | 181 ± 5 | 2.0 ± 0.1 |
| Res E-l | 201 ± 4 | 8.6 ± 0.3 |
| Res N-l | 174 ± 4 | 2.3 ± 0.1 |
| Res W-l | 235 ± 9 | 1.3 ± 0.1 |
|
|
||
| CrA point-source average | 197 ± 9 b | 3.1 ± 1.6 b |
| CrA extended average | 198 ± 12 b | 3.5 ± 1.5 b |
|
|
||
| NGC 1333 IRAS 4Bc | 110/220 | 100 |
| Serpens SMM1d | 136 ± 27 | ... |
| Serpens SMM3/4 averagee | 105 ± 6 b | 25 ± 3 b |
|
|
||
| DIGITf | 194 ± 20 b | 7.7 ± 2.6 b |
Notes.
The methods used for calculating the error estimates are the same as for the CO rotational diagrams, see Sects. 4.2.1 and 4.2.2.
For the sample averages, standard deviations of the mean of the significant fits are given (see Table 5).
From Herczeg et al. (2012). Two separate cool and warm components.
From Goicoechea et al. (2012).
Average of SMM3b, SMM3c, SMM3r, and SMM4, from Dionatos et al. (2013), assuming a distance of 415 pc.
Average of the DIGIT sample, from Green et al. (2013), not including the CrA and Serpens sources.
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