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Table 3

Fundamental parameters and wind properties for the stars in our sample.

Star Teff log gc log () v β f vcl vsin   i vmac Mspec Age
HD [kK] [km s-1] [km s-1] [km s-1] [km s-1] [M] [M] [M] [Myr]

16691 41.0 3.66 5.94  −5.52 2300 1.2 0.06 130 135 37 56.6 53.4 65.2 3.1
66811 40.0 3.64 5.91  −5.70 2300 0.9 0.05 100 210 90 56.1 51.1 62.3 3.2
190429A 39.0 3.62 5.96  −5.68 2300 1.0 0.04 30 150 57 66.0 54.6 68.0 3.3
15570 38.0 3.51 5.94  −5.66 2200 1.1 0.05 30 97 40 54.0 48.7 59.5 3.4
14947 37.0 3.52 5.83  −5.85 2300 1.3 0.03 30 130 36 48.0 43.4 51.2 3.9
210839 36.0 3.54 5.80  −5.85 2100 1.0 0.05 120 210 80 51.4 42.3 50.5 4.0
163758 34.5 3.41 5.76  −5.80 2100 1.1 0.05 30 94 34 41.6 41.2 48 0 4.1
192639 33.5 3.42 5.68  −5.92 1900 1.3 0.05 30 90 43 38.3 39.1 43. 0 4.2

Notes. Mspec, , refer to spectroscopic mass, initial mass and mass at the corresponding stellar age, respectively. Uncertainties for Teff are  ± 1000 K,  ± 0.1 dex for log g and  ± 0.1 dex on log L/L (reflecting the uncertainty on the distance). An uncertainty of  ± 0.2  ×    10-6 M yr-1 was estimated for the mass-loss rates. v is measured within  ± 100 km s-1.

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