Table A.2
Results for the 12CO 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 | 0.68 | 20 | −23 | 21 | 0.5 | 0.52 | Low S/N |
| 2 - OH358.162+0.490 | 9.4 | 320 | 4 | 26 | 0.5 | 0.70 | |
| 3 - OH358.235+0.115 | 0.91 | 32 | −21 | 19 | 0.0 | 0.46 | Low S/N |
| 4 - OH358.505+0.330 | 2.2 | 57 | −34 | 27 | −0.2 | … | Low S/N |
| 5 - OH359.140+1.137 | 0.26 | 5.2 | −134 | 13 | 0.0 | … | B > 25 m data used |
| 6 - OH359.149−0.043 | 2.0 | 57 | 47 | 27 | 1.0 | … | B >25 m data used; Brightness distr.? |
| 7 - OH359.220+0.163 | 2.1 | 40 | −139 | 13 | 0.5 | 1.26 | Brightness distr.? |
| 8 - OH359.233−1.876 | 0.65 | 15 | −11 | 21 | 0.5 | 0.31 | Low S/N |
| 9 - OH359.467+1.029 | 0.74 | 18 | 110 | 15 | 0.5 | 0.58 | Low S/N |
| 10 - OH359.543−1.775 | 0.18 | 8.4 | 90 | 37 | 0.5 | 0.27 | Low S/N |
| 11 - OH359.664+0.636 | 0.28 | 4.8 | −158 | 14 | 0.5 | … | Low S/N |
| 12 - OH359.745−0.404 | 0.25 | 6.4 | 189 | 20 | 0.5 | … | B >25 m data used; Low S/N |
| 13 - OH359.805+0.200 | <0.3 | … | … | … | … | … | |
| 14 - OH359.826+0.153 | 0.25 | 6.7 | −26 | 19 | 0.0 | … | |
| 15 - OH359.902+0.061 | 0.29 | 6.5 | −129 | 11 | 0.5 | 0.24 | Low S/N |
| 16 - OH0.173+0.211 | <0.6 | … | … | … | … | … | |
| 17 - OH0.221+0.168 | 0.85 | 13 | 66 | 15 | 0.5 | 0.31 | B >25 m data used; Low S/N |
| 18 - OH0.548−0.059 | 0.45 | 8.6 | −47 | 23 | 0.0 | 0.35 | B >50 m data used; Low S/N |
| 19 - OH0.739+0.411 | 1.3 | 27 | −21 | 15 | 0.5 | 0.33 | B > 25 m data used |
| 20 - OH1.095−0.832 | 1.8 | 86 | 11 | 22 | 0.0 | 0.83 | |
| 21 - OH1.221+0.294 | 3.0 | 43 | −261 | 10 | 0.5 | … | |
| 22 - OH1.628+0.617 | 0.45 | 15 | −87 | 25 | 0.0 | … |
Notes. (a) The upper limits are 3σ. See text for details on the uncertainties of the flux densities, but we estimate that for lines stronger than 2.0 Jy the uncertainty is about 10%, while for lines weaker than 1.0 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 ± 3 and ± 2 km s−1, respectively.(c) Average of the deconvolved major and minor axes of a two-dimensional Gaussian fit to the brightness distribution.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.