Time-dependent models for magnetic CP stars. V - The oblique rotator

Details Time-dependent models for magnetic CP stars. V - The oblique rotator Time-dependent models for magnetic CP stars. V - The oblique rotator

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.244..272m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 244, May 15, 1990, p. 272-280.

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18

Astronomical Models, Magnetic Stars, Main Sequence Stars, Stellar Evolution, Time Dependence, Computational Astrophysics, Stellar Envelopes, Stellar Magnetic Fields, Stellar Mass, Stellar Rotation

Scientific paper

A fully three-dimensional code for magnetic CP stars is introduced that follows the evolution of the magnetic field of the star simultaneously with the evolution of the thermal structure of the stellar model. The nuclear evolution of the stellar model is not included, although estimates of evolutionary effects are given. The model is used to calculate the evolution of the large-scale magnetic fields immersed in the radiative envelopes of middle main-sequence stars over time-scales comparable with the main-sequence lifetimes of the stars.

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