Rotationally-modulated photometric variations of magnetic CP stars - theoretical aspects

Details Rotationally-modulated photometric variations of magnetic CP stars - theoretical aspects Rotationally-modulated photometric variations of magnetic CP stars - theoretical aspects

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coska..38..369k&link_type=abstract

Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2, p. 369-374.

Other

Stars: Chemically Peculiar, Stars: Early-Type, Stars: Variables: Other, Stars: Atmospheres, Stars: Magnetic

Scientific paper

We study theoretical aspects of the light variability of magnetic chemically-peculiar stars, using HD37776 and HR7224 as the test cases for our understanding of the light variability. We are able to reproduce their light curves from the known distribution of surface elements. We show that the light variability of these stars is mainly due to the inhomogeneous surface distribution of overabundant silicon, iron and helium.

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