Table 5
CO rotational temperatures and total number of molecules.
| YSO | T warm a |
a
|
T hot a |
a
|
| [K] | [1048] | [K] | [1048] | |
|
|
||||
| IRS7A+SMM 1Cb | 294 ± 16 | 33.0 ± 3.0 | 682 ± 34 | 2.7 ± 0.3 |
| IRS7B | 273 ± 14 | 12.0 ± 1.1 | 710 ± 54 | 0.51 ± 0.07 |
| R CrA | 287 ± 16 | 5.4 ± 0.5 | 992 ± 91 | 0.27 ± 0.03 |
| IRS5A | 293 ± 17 | 3.1 ± 0.3 | 1417 ± 780 | 0.12 ± 0.04 |
| IRS5N | 283 ± 24 | 0.7 ± 0.1 | ... | ... |
|
|
||||
| Res SW-l |
|
5.0 ± 0.5 |
|
0.35 ± 0.06 |
| Res E-l |
|
1.7 ± 0.2 | 1015 ± 198 | 0.09 ± 0.02 |
| Res N-l |
|
3.3 ± 0.3 | 898 ± 334 | 0.11 ± 0.06 |
| Res W-l |
|
13.0 ± 1.2 |
|
0.40 ± 0.07 |
|
|
||||
| CrA point-source average | 286 ± 3 c | 10.8 ± 5.2 c | 950 ± 148 c | 0.90 ± 0.52 c |
| CrA extended average | 277 ± 7 c | 5.8 ± 2.2 c | 829 ± 69 c | 0.24 ± 0.07 c |
|
|
||||
| NGC 1333 IRAS 4Bd | 280 | 40 | 880 | 3 |
| Serpens SMM1e | 337 ± 40 | ... | 622 ± 30 | ... |
| Serpens SMM3/4 averagef | 260 ± 10 c | 49 ± 6 c | 800 ± 60 c | 2.2 ± 0.6 c |
|
|
||||
| DIGIT averageg | 355 ± 3 c | 5.2 ± 0.4 c | 814 ± 29 c | 1.63 ± 0.20 c |
| HOPS averageh | 288 ± 14 c | ... | 735 ± 37 c | ... |
Notes.
The separation between these sources is too small to allow treating their line fluxes independently using POMAC.
For the sample averages, standard deviations of the mean (the standard deviation of the sample divided by the square root of the sample size) of the significant fits are given.
From Herczeg et al. (2012).
From Goicoechea et al. (2012).
Average of SMM3b, SMM3c, SMM3r, and SMM4, from Dionatos et al. (2013), assuming a distance of 415 pc.
From Green et al. (2013), including all DIGIT embedded sources except the CrA and Serpens SMM3/4 sources. The Serpens region is, like the CrA region, affected by confusion and is treated in a separate paper (Dionatos et al. 2013).
From Manoj et al. (2013).
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