Free Access

Table 4

Stellar wind parameters.

T v β R X(C) X(N) X(O)
kK km s-1 R 10-6   M yr-1

This work 401 2300 1 17.3 3.5 6.00 × 10-4 7.7 × 10-3 3.05 × 10-3

Bouret et al. (2012) 40 2300 0.9 17.3 2.00 2.86 × 10-4 1.05 × 10-2 1.30 × 10-3

Pauldrach et al. (2012) 39 2100 19 13.7 8.2 × 10-3 9.13 × 10-3 1.14 × 10-3

Notes. The CNO abundances are given as mass fractions. Note that Pauldrach et al. (2012) did not assume a β-law for the wind velocity, but performed a full hydrodynamical computation of the wind.

(1)

We cannot determine the effective temperature of the star with our code. Because this parameter is important for the mass absorption coefficient calculation, we indicate the value we adopted in our analysis.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.