Table 8
Observed continuum fluxes at 5 GHz of H ii regions, obtained from the literature, that are ionized by clusters (including the overall Dragonfish nebula), together with derived ionizing fluxes at 12.4 kpc.
| H ii region | Embedded population | l (°) | b (°) | fν [Ref.] | QH (12.4 kpc) |
|
|
|||||
| GAL 297.51-0.77 | La Serena 19/20; Mercer 29 | 297.506 | −0.765 | 3.5 Jy [1] | 8.6 × 1049 s-1 |
| GAL 297.66-0.98 | La Serena 22; New candidate | 297.655 | −0.977 | 1.6 Jy [1] | 3.9 × 1049 s-1 |
| GAL 298.19-0.78 | DBSB 75 | 298.187 | −0.782 | 2.4 Jy [1] | 5.9 × 1049 s-1 |
| GAL 298.23-0.33 | DBSB 74 | 298.228 | −0.331 | 47.4 Jy [2] | 1.159 × 1051 s-1 |
| GAL 298.56-0.11 | Filament of YSOs | 298.559 | −0.114 | 2.8 Jy [1] | 6.8 × 1049 s-1 |
| WMG70 298.8-0.3 | DBSB 129 | 298.838 | −0.347 | 16.0 Jy [4] | 3.91 × 1050 s-1 |
| GAL 298.87-0.43 | Mercer 31 | 298.868 | −0.423 | 42.4 Jy [2] | 1.037 × 1051 s-1 |
| GAL 299.02+0.15 | G3CC 2 | 299.016 | +0.148 | 2.6 Jy [1] | 6.4 × 1049 s-1 |
|
|
|||||
| Dragonfish Nebula | 298.4 | −0.4 | ≲312 Jy [3]a | ≲ 7.63 × 1051 s-1 | |
Notes.
The original estimate of 313 Jy has been slightly modified to account for the almost negligible foreground contribution (see text).
Reference. (1) Caswell & Haynes (1987); (2) Conti & Crowther (2004); (3)Murray & Rahman (2010); (4) Wilson et al. (1970).
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