Table 3
Radiative flux of the recombination lines from central region.
| Source | ƒBrγ(P < 1″) | ƒH30α(P < 1″) | ƒBrγ(p < 0.23″) | ƒH30α(p < 0.23″) |
|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) |
| Observed | – | – | ≤7.26 × 10−15 | (3.0 ± 0.6) × 10−17 |
| WR_f07 | 6.08 × 10−17 | 6.70 × 10−22 | 1.18 × 10−18 | 1.34 × 10−27 |
| WR_f1 | 5.74 × 10−13 | 2.19 × 10−17 | 5.32 × 10−13 | 2.05 × 10−17 |
Notes. All fluxes correspond to quantities seen from Earth, i.e. at a distance of 8.33 kpc, and are given in units erg cm−2 s−1. The observed H30ɑ flux was calculated integrating the reported flux density across the velocity channels, and taking into consideration the error propagation of the 0.3 mJy reported (see Fig. 1 in Murchikova et al. 2019).
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