Table 6
OH rotational temperatures and total number of molecules.
| YSO | T a |
a
|
| [K] | [1045] | |
|
|
||
| IRS7A+SMM 1C | 83 ± 3 | 132 ± 12 |
| IRS7B | 89 ± 4 | 16.7 ± 1.5 |
| R CrA | 99 ± 5 | 7.1 ± 0.7 |
| IRS5A | 80 ± 3 | 17.2 ± 1.5 |
|
|
||
| Res SW-l | 76 ± 4 | 9.5 ± 1.1 |
| Res E-l | 68 ± 4 | 7.2 ± 1.2 |
| Res N-l | 66 ± 2 | 19.1 ± 2.1 |
| Res W-l | 72 ± 2 | 26.1 ± 2.5 |
|
|
||
| CrA point-source average | 88 ± 4 b | 43.3 ± 25.7 b |
| CrA extended average | 71 ± 2 b | 15.5 ± 3.8 b |
|
|
||
| NGC 1333 IRAS 4Bc | 60 | 130 |
| Serpens SMM1d | 72 ± 8 | ... |
| Serpens SMM3/4 averagee | 88 ± 2 b | 26 ± 3 b |
|
|
||
| DIGITf | 83 ± 3 b | 24 ± 3 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). Only the cool component based chiefly on PACS data is given here.
From Wampfler et al. (2013).
Average of SMM3b and SMM4, from Dionatos et al. (2013), assuming a distance of 415 pc. This value is calculated excluding the same lines that have been excluded in this paper, and does not agree with the values given in Dionatos et al. (2013) for this reason.
Average of the DIGIT sample, from Green et al. (2013), not including the CrA and Serpens sources. This value is calculated excluding the same lines that have been excluded in this paper, and for this reason does not agree with the value given in Green et al. (2013) (183 K).
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