Really focused stellar winds in X-ray binaries | Astronomy & Astrophysics (A&A)

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Fig. 2

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Distribution of the stellar wind intensity in dependence on gravity darkening. The radial approximation for the same parameters as in Fig. 1 is calculated for radiation modulated according to Eq. (10) and values of the parameter β from the top to the bottom of 0.0, 0.125, 0.1875, and 0.25.

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