Table A.3
Results for the 13CO J = 3–2 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 | 0.18 | 6.4 | −26 | 26 | 0.5 | 0.37 | |
| 2 - OH358.162+0.490 | 1.7 | 74 | 2 | 23 | 0.0 | 0.72 | |
| 3 - OH358.235+0.115 | 0.04 | 2.2 | −17 | 18 | 0.0 | 0.16 | Low S/N |
| 4 - OH358.505+0.330 | 0.91 | 25 | −26 | 20 | 0.5 | 0.93 | Resolved structure |
| 5 - OH359.140+1.137 | 0.19 | 3.1 | −135 | 12 | 0.5 | 0.27 | |
| 6 - OH359.149−0.043 | 0.28 | 3.1 | 46 | 25 | 1.0 | … | B >25 m data used; Brightness distr.? |
| 7 - OH359.220+0.163 | 0.51 | 16 | −135 | 19 | 0.3 | 0.72 | Resolved structure |
| 8 - OH359.233−1.876 | 0.24 | 6.3 | −15 | 18 | 0.5 | 0.28 | |
| 9 - OH359.467+1.029 | 0.10 | 2.8 | 110 | 23 | 0.5 | 0.43 | |
| 10 - OH359.543−1.775 | 0.13 | 6.7 | 87 | 40 | 0.5 | 0.24 | Line profile? |
| 11 - OH359.664+0.636 | 0.10 | 1.9 | −157 | 13 | 0.5 | 0.35 | |
| 12 - OH359.745−0.404 | 0.13 | 3.9 | 186 | 20 | 0.5 | 0.34 | |
| 13 - OH359.805+0.200 | 0.05 | 1.4 | −51 | 21 | 0.3 | 0.32 | Low S/N |
| 14 - OH359.826+0.153 | 0.05 | 1.5 | −25 | 16 | 0.0 | 0.35 | Low S/N |
| 15 - OH359.902+0.061 | 0.06 | 2.2 | −133 | 19 | 0.0 | 0.37 | B >25 m data used; Low S/N |
| 16 - OH0.173+0.211 | <0.08 | … | … | … | … | … | |
| 17 - OH0.221+0.168 | 0.05 | 1.9 | 67 | 27 | 1.0 | 0.36 | B >25 m data used; Low S/N |
| 18 - OH0.548−0.059 | 0.15 | 6.0 | −45 | 31 | 0.5 | 0.37 | B >50 m data used; Line profile? |
| 19 - OH0.739+0.411 | 0.58 | 9.2 | −21 | 10 | 0.5 | 0.50 | Line profile? |
| 20 - OH1.095−0.832 | 0.60 | 33 | 12 | 33 | −0.3 | 0.64 | |
| 21 - OH1.221+0.294 | 0.11 | 4.1 | −258 | 17 | 0.0 | 0.31 | |
| 22 - OH1.628+0.617 | 0.03 | 2.1 | −87 | 25 | −0.3 | 0.22 | Low S/N |
Notes. (a) The upper limit is 3σ. See text for details on the uncertainties of the flux densities, but we estimate that for lines stronger than 0.2 Jy the uncertainty is about 10%, while for lines weaker than 0.1 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 ± 1.5 and ± 1 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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