Table A.1
Results for the 12CO J = 2–1 line.
| Source | S (a) [Jy] | ∫S dv [Jy km s−1] | vc(b) [km s−1] | v∞(b) [km s−1] | β | θs(c) [″] | Remarks |
|---|---|---|---|---|---|---|---|
| 1 - OH358.083+0.137 | 0.35 | 8.7 | −24 | 19 | 0.5 | 0.38 | Low S/N |
| 2 - OH358.162+0.490 | 6.0 | 250 | 3 | 20 | 0.0 | 1.46 | |
| 3 - OH358.235+0.115 | 0.45 | 14 | −25 | 19 | 0.0 | 0.63 | |
| 4 - OH358.505+0.330 | 1.5 | 31 | −30 | 25 | −0.5 | 0.70 | B >25 m data used |
| 5 - OH359.140+1.137 | 0.78 | 12 | −137 | 11 | 0.5 | 0.44 | |
| 6 - OH359.149−0.043 | 0.31 | 11 | 53 | 27 | 1.0 | … | B >50 m data used; Brightness distr.? |
| 7 - OH359.220+0.163 | 2.3 | 50 | −138 | 15 | 0.5 | 1.25 | Resolved structure |
| 8 - OH359.233−1.876 | 0.98 | 23 | −16 | 17 | 0.5 | 0.60 | |
| 9 - OH359.467+1.029 | 0.30 | 11 | 110 | 16 | 0.5 | 0.58 | |
| 10 - OH359.543−1.775 | 0.15 | 7.3 | 95 | 32 | 0.5 | 0.31 | Low S/N |
| 11 - OH359.664+0.636 | 0.91 | 16 | −158 | 13 | 0.5 | 0.84 | |
| 12 - OH359.745−0.404 | 0.44 | 9.9 | 184 | 22 | 0.5 | 0.69 | |
| 13 - OH359.805+0.200 | 0.22 | 2.9 | −48 | 15 | 0.3 | … | B >25 m data used; Low S/N |
| 14 - OH359.826+0.153 | 0.12 | 2.5 | −26 | 16 | 0.3 | 0.51 | B >50 m data used; Low S/N |
| 15 - OH359.902+0.061 | 0.51 | 8.4 | −123 | 13 | 0.5 | 0.43 | B >25 m data used; Low S/N |
| 16 - OH0.173+0.211 | 0.31 | 7.5 | 52 | 18 | 1.0 | 0.52 | B >25 m data used |
| 17 - OH0.221+0.168 | 0.13 | 4.9 | 60 | 26 | 1.0 | 0.44 | B >50 m data used |
| 18 - OH0.548−0.059 | 0.10 | 2.0 | −53 | 22 | −0.5 | 0.59 | B >50 m data used; Low S/N |
| 19 - OH0.739+0.411 | 0.81 | 13 | −21 | 12 | 0.3 | 1.04 | B >25 m data used; Line profile? |
| 20 - OH1.095-0.832 | 2.1 | 104 | 10 | 23 | −0.3 | 0.91 | |
| 21 - OH1.221+0.294 | 2.2 | 44 | −261 | 14 | 0.5 | 0.57 | |
| 22 - OH1.628+0.617 | 0.86 | 34 | −84 | 30 | 1.0 | 0.80 |
Notes. (a) See text for details on the uncertainties of the flux densities, but we estimate that for lines stronger than 1.0 Jy the uncertainty is about 10%, while for lines weaker than 0.4 Jy the uncertainty increases to about 50% for the weakest lines.(b) The uncertainties in the expansion and centre velocities are estimated to be about ± 2 and ± 1.5 km s−1, respectively.(c) Average of the deconvolved major and minor axes of a two-dimensional Gaussian fit to the brightness distribution.
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