Table 8.
Mass-loss estimates for YHGs and RSGs.
| Source | Spectral type | ATCA  (M⊙ yr−1) |
|---|---|---|
| W12a | F1Ia+ | 1.66 ± 0.02 × 10−5 |
| W4a | F3Ia+ | 2.59 ± 0.02 × 10−5 |
| W32 | F5Ia+ | 3.01 ± 0.50 × 10−6 |
| W265 | F5Ia+ | 1.10 ± 0.03 × 10−5 |
| W237 | M3Ia | 2.00 ± 0.02 × 10−6 |
| W75 | M4Ia | 7.27 ± 0.48 × 10−7 |
| W20 | M5Ia | 3.28 ± 0.03 × 10−6 |
Notes. Fluxes were used from core components of the emission attributed to the YHGs and RSGs, as given by the FULLCONCAT dataset. These mass-loss rates are calculated for objects where an approximation of a thermally emitting stellar wind is considered valid, using the Wright and Barlow equation (Wright & Barlow 1975).
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