Table 9:
Comparison of sources detected at 8.6 GHz in this survey and in the methanol maser survey of Walsh et al. (1998). (The peak fluxes for the methanol maser survey have been taken from Walsh et al. (1998), however, the integrated fluxes were not presented in their paper but are available from VizieR http://vizier.u-strasbg.fr/viz-bin/VizieR).
| |
RMS survey |
Walsh et al. (1998) |
| RMS name |
Peak |
Integ. |
Peak |
Integ. |
| G268.4222-0.8490 |
307.1 |
1696.0 |
510 |
1012.0 |
| G305.1967+0.0335 |
113.1 |
1105.0 |
90 |
394.0 |
| G318.9148-0.1647 |
60.6 |
1659.0 |
120 |
424.0 |
| G330.9544-0.1817 |
591.8 |
1728.0 |
280 |
1161.0 |
| G337.7051-0.0575 |
152.8 |
171.0 |
84 |
94.0 |
| G344.4257+0.0451 |
63.5 |
268.3 |
28 |
485.0 |
| G345.0061+1.7944 |
189.9 |
209.0 |
140 |
130.0 |
| G345.4881+0.3148 |
456.9 |
2163.0 |
200 |
2100a |
| G346.5234+0.0839 |
77.0 |
150.3 |
45 |
104.0 |
| G348.6972-1.0263 |
402.2 |
1194.0 |
500 |
843.0 |
a The integrate flux for this source obtained from VizieR is incorrect (48.4 mJy),
the correct flux was provided by Andrew Walsh (private com.).
|
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