Stellar Winds and Mass Loss of a Rotating Star

Details Stellar Winds and Mass Loss of a Rotating Star Stellar Winds and Mass Loss of a Rotating Star

Sep 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..18..128d&link_type=abstract

Astrophysics and Space Science, Volume 18, Issue 1, pp.128-134

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

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% forv rot up to 200 km s-1.

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