|Spectral Type||B1IVe shell||fixed||2, 3|
|Weak line force||Free||1|
|a References: 1) this work; 2) Paper I; 3) Yang et al. (1990); 4) Harmanec (1988); 5) Cranmer (2005); 6) Perryman et al. (1997); 7) Harmanec (1984); b was calculated from and for a rigidly rotating star in the Roche approximation; c the equatorial temperature, , was calculated from and for a rigidly rotating star in the Roche approximation; d M was calculated from ; e corresponds to the average effective temperature of a rotationally deformed, gravity darkened star; f H0 was calculated from Eq. (8), assuming a mean molecular weight of 0.6 and an electron temperature of after Carciofi & Bjorkman (2006); g is given by (Eq. (10)); h d was considered a free parameter within the 113-148 pc range, corresponding to the accuracy in the distance determination the Hipparcos satellite.|
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