Table 5
Radio (5 GHz) flux of each HII region and spectral α (updated from Urquhart et al. (2014)).
| Source | S5GHz | α | Stot | SFF | Sdust | Mdust |
|---|---|---|---|---|---|---|
| G302.02 | 59.5 | –0.03 | 62.1 | 53.2 | 8.9 | 29.6 |
| G302.48 | 23.4 | 0.03 | 93.9 | 26.2 | 67.7 | 142.4 |
| G309.89 | 1.2 | – | 36.3 | – | – | – |
| G330.28 | 44.9 | –0.08 | 79.9 | 33.3 | 46.6 | 253.5 |
| G332.77 | 24.6 | – | 3.5 | – | – | – |
| G336.98 | 18.0 | 0.52 | 243.9 | 126.7 | 117.1 | 312.8 |
| G337.63 | 31.0 | 0.01 | 53.1 | 32.2 | 20.9 | 33.9 |
| G337.84 | 11.1 | 0.63 | 135.3 | 118.1 | 17.2 | 68.5 |
| G339.11 | 42.9 | –0.04 | 189.3 | 36.9 | 152.4 | 686.0 |
Notes. The total flux from the HII region bearing Fellwalker core (Stot ) is subsequently listed as a reminder from Table A.2 because the free-free extrapolated flux (SFF ) is then removed from the 256 GHz continuum flux to give the expected contribution to the continuum emission (Sdust ). All fluxes are listed in units of mJy. Using the dust mass assumptions described in Sect. 3.1.3 and a temperature of 70 K, the resultant dust masses are presented in units of M⊙ .
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