Table 7
Mechanical wind properties of the sample stars.
| Star – | Sp. type – | υ∞ km s−1 | log Ṁ M⊙/yr | C06 | L07 | S08 | K15 | H18 | R22 |
|---|---|---|---|---|---|---|---|---|---|
| HD206165 | B2Ib | 900 | −6.671.0 | − | − | -6.301−6.37 | − | − | − |
| HD198478 | B2.5Ia | 570 | −6.141.0 | −6.631−6.19 | − | −6.301-5.94 | -6.621−6.01 | − | ≲−6.42|≲-5.90 |
| HD53138 | B3Ia | 680 | −6.630.5 | −6.441−6.63 | −6.511−6.46 | −6.341−6.46 | − | −6.621−6.65 | ≲-5.74|≲-5.93 |
| HD164353 | B5Ib/II | 640 | −8.150.5 | − | − | -7.221−7.36 | − | − | − |
Notes. For comparison, we also show literature results. Boldface values indicate the mass-loss rates re-scaled to the radii we obtained for each BSG. Subscripts indicate the chosen clumping values. C06 stands for Crowther et al. (2006), L07 for Lefever et al. (2007), S08 for Searle et al. (2008), K15 for Kraus et al. (2015), H18 for Haucke et al. (2018), and R22 for Rubio-Diez et al. (2022).
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