Table 2
Summary of the observational data sets of the globule.
| Instrument | Species | λ | ν | Δ v | Θ |
|---|---|---|---|---|---|
| [μm] | [GHz] | [km s−1] | [″] | ||
| Herschel spectroscopy | |||||
| HIFI | [C II] | 157.7 | 1900.5 | 0.7 | 12.2 |
| PACS | [C II] | 157.7 | 1900.5 | − | ~11 |
| PACS | [O I] | 145.5 | 2060.1 | − | ~10 |
| PACS | [O I] | 63.2 | 4744.8 | − | ~9.5 |
| PACS | [N II] | 121.9 | 2459.3 | − | ~9.4 |
| PACS | 12CO 16→15 | 162.8 | 1841.4 | − | ~11.5 |
| PACS | 12CO 14→13 | 186.0 | 1611.8 | − | ~12.5 |
| PACS | 12CO 13→12 | 200.3 | 1496.9 | − | ~13 |
| SPIRE | [C I] | 370.4 | 809.3 | − | 34.8 |
| SPIRE | [C I] | 609.1 | 492.2 | − | 37.2 |
| SPIRE | [N II] | 205.2 | 1461.1 | − | 16.9 |
| SPIRE | 12CO 13→12 | 200.3 | 1496.9 | − | 16.8 |
| SPIRE | 12CO 12→11 | 216.9 | 1382.0 | − | 17.2 |
| SPIRE | 12CO 11→10 | 236.6 | 1267.0 | − | 17.6 |
| SPIRE | 12CO 10→9 | 260.2 | 1152.0 | − | 17.7 |
| SPIRE | 12CO 9→8 | 289.1 | 1036.9 | − | 19.2 |
| SPIRE | 12CO 8→7 | 325.2 | 921.8 | − | 36.8 |
| SPIRE | 12CO 7→6 | 371.7 | 806.7 | − | 34.8 |
| SPIRE | 12CO 6→5 | 433.6 | 691.5 | − | 29.4 |
| SPIRE | 12CO 5→4 | 520.3 | 576.3 | − | 32.6 |
| SPIRE | 12CO 4→3 | 650.3 | 461.0 | − | 40.4 |
| SPIRE | 13CO 9→8 | 302.4 | 988.8 | − | 36.1 |
| SPIRE | 13CO 8→7 | 340.2 | 881.3 | − | 36.1 |
| SPIRE | 13CO 7→6 | 388.7 | 771.2 | − | 34.0 |
| SPIRE | 13CO 6→5 | 453.5 | 661.1 | − | 30.0 |
| SPIRE | 13CO 5→4 | 544.2 | 550.9 | − | 32.9 |
| Herschel photometry | |||||
| PACS | Continuum | 70 | 4283 | − | 6.0 |
| PACS | Continuum | 160 | 1874 | − | 11.4 |
| SPIRE | Continuum | 250 | 1199 | − | 17.8 |
| SPIRE | Continuum | 350 | 857 | − | 25.0 |
| SPIRE | Continuum | 500 | 600 | − | 35.7 |
| SOFIA | |||||
| GREAT | [C II] | 157.74 | 1900.5 | 0.23 | 15.1 |
| GREAT | 12 CO 11→10 | 236.61 | 1267.0 | 0.69 | 22.5 |
| upGREAT | [O I] | 63.18 | 4744.8 | 0.25 | 6.1 |
| upGREAT | 12 CO 16→15 | 162.81 | 1841.4 | 0.64 | 15.3 |
| FCRAO | |||||
| SEQUOIA | 13 CO 1→0 | 2720.4 | 110.2 | 0.067 | 45 |
| SEQUOIA | CS 2→1 | 3059.1 | 98.0 | 0.075 | 48 |
| JCMT | |||||
| HARP | 12 CO 3→2 | 869.0 | 345.8 | 0.42 | 15 |
Notes. The first column gives the instrument, the second the line (or continuum), the third and forth the wavelength and frequency, the fifth the velocity resolution used in this paper, and the six column the angular resolution. We note that the PACS and SPIRE FIR lines are not spectrally resolved and that the SOFIA and FCRAO line observations were smoothed to a lower velocity resolution when used in displays of spectral line maps or channel maps. For PDR-modelling, we smoothed all data sets with an angular resolution higher than 20″ to a common value of 20″.
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