The effect of rotation on the luminosity of magnetic stars

Details The effect of rotation on the luminosity of magnetic stars The effect of rotation on the luminosity of magnetic stars

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.100..219s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 100, no. 1-2, March 1984, p. 219-225.

Astronomy and Astrophysics

Astrophysics

Magnetic Stars, Main Sequence Stars, Stellar Luminosity, Stellar Rotation, Magnetic Field Configurations, Perturbation Theory, Poloidal Flux, Radii, Stellar Magnetic Fields, Stellar Models, Stellar Temperature

Scientific paper

The effect of rotation and a general magnetic field on the luminosity, radius, and effective temperature of the upper Main-Sequence stars has been investigated using a perturbation analysis. The magnetic field profile prevailing inside the star is assumed to have both poloidal and toroidal components. The case of constant as well as differential rotation is admitted. Model calculations indicate that these stellar parameters modify considerably as a result of coupling between rotation and the magnetic field.

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