Stellar winds and mass loss of a rotating star |
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| Authors: | J. P. De Grève C. De Loore C. De Jager |
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| Affiliation: | (1) The Astrophysical Institute, Brussels, Belgium;(2) The Astronomical Institute, Utrecht, Holland |
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| Abstract: | The mass loss to be expected from the corona of a rotating F2-star is calculated. The rotation is supposed to be rigid up to a certain distances, as if it were maintained by a strong magnetic field. Dependent on the values of the rotational velocity the mass loss can increase to 26–40% forvrot up to 200 km s–1. |
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