Table 2
Summary of averaged integrated intensities and spatial offsets of the observations.
Transition | Frequencya | Observatory | Beamsizeb | Peak intensityc | y-offsetd | y-offsetd | Δyobs e |
[GHz] | [arcsec] | [K km s-1] | [pc] | [arcsec] | [pc] | ||
|
|||||||
[Cii] | 1900.5369 | HIFI/Herschel | 11.2 | 1153 ± 115 | −0.016 ± 0.005 | −7.8 ± 2.4 | 0 |
CO 2−1 | 230.5380000 | CSO | 30.5 | 402 ± 32 | 0.029 ± 0.006 | 14.6 ± 3.0 | 0.045 ± 0.008 |
CO 3−2 | 345.7959899 | CSO | 21.9 | 406 ± 68 | 0.014 ± 0.006 | 7.2 ± 3.0 | 0.030 ± 0.008 |
CO 6−5 | 691.4730763 | CSO | 10.6 | 560 ± 244 | 0.020 ± 0.006 | 9.8 ± 3.0 | 0.036 ± 0.008 |
CO 10−9 | 1151.985452 | HIFI/Herschel | 18.4 | 374 ± 37 | 0.021 ± 0.005 | 10.5 ± 2.4 | 0.037 ± 0.007 |
CO 16−15 | 1841.345506 | HIFI/Herschel | 11.5 | 128 ± 13 | 0.019 ± 0.005 | 9.4 ± 2.4 | 0.035 ± 0.007 |
13CO 3−2 | 330.5879653 | CSO | 21.9 | 114 ± 18 | 0.026 ± 0.006 | 12.8 ± 3.0 | 0.042 ± 0.008 |
13CO 5−4 | 550.9262851 | HIFI/Herschel | 38.5 | 120 ± 12 | 0.042 ± 0.005 | 20.8 ± 2.4 | 0.058 ± 0.007 |
13CO 6−5 | 661.0672766 | CSO | 10.6 | 157 ± 65 | 0.030 ± 0.006 | 14.8 ± 3.0 | 0.046 ± 0.008 |
13CO 10−9 | 1101.3495971 | HIFI/Herschel | 19.3 | 92 ± 9.2 | 0.018 ± 0.005 | 9.0 ± 2.4 | 0.034 ± 0.007 |
HCO+3−2 | 267.5576259 | CSO | 30.5 | 46 ± 5 | 0.010 ± 0.006 | 5.0 ± 3.0 | 0.026 ± 0.008 |
HCO+6−5 | 535.0615810 | HIFI/Herschel | 39.6 | 8.7 ± 0.87 | 0.022 ± 0.005 | 11.2 ± 2.4 | 0.038 ± 0.007 |
Notes.
Taken from The Cologne Database for Molecular Spectroscopy (CMDS) (Müller et al. 2001, 2005; http://www.astro.uni-koeln.de/cdms/).
Calculated based on Roelfsema et al. (2012) for HIFI/Herschel. Taken from http://www.submm.caltech.edu/cso/receivers/beams.html (calculated FWHM) for CSO data. For non-circular beams an average has been used.
Line-integrated intensity averaged along the bar at the position of the peak (see text), Tmb scale. For HIFI/Herschel the error on Tmb is about 10% (see Roelfsema et al. 2012). The error given for the CSO data has been calculated (and extrapolated for frequencies >345 GHz) based on the errors on and ηmb given in Mangum (1993).
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