Advanced test of the model stellar atmospheres: the nature of the light variability of magnetic chemically peculiar stars

Details Advanced test of the model stellar atmospheres: the nature of the light variability of magnetic chemically peculiar stars Advanced test of the model stellar atmospheres: the nature of the light variability of magnetic chemically peculiar stars

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..252..347k&link_type=abstract

The Art of Modeling Stars in the 21st Century, Proceedings of the International Astronomical Union, IAU Symposium, Volume 252, p

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

Scientific paper

The magnetic chemically peculiar stars exhibit both inhomogeneous horizontal distribution of chemical elements on their surfaces and the light variability. We show that the observed light variability of these stars can be successfully simulated using models of their stellar atmospheres and adopting the observed surface distribution of elements. The most important elements that influence the light variability are silicon, iron, and helium.

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