Model atmospheres of magnetic and chemically peculiar stars

Details Model atmospheres of magnetic and chemically peculiar stars Model atmospheres of magnetic and chemically peculiar stars

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coska..38..267k&link_type=abstract

Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2, p. 267-272.

Astronomy and Astrophysics

Astronomy

Stars: Chemically Peculiar, Stars: Atmospheres, Stars: Magnetic Fields, Stars: Abundances

Scientific paper

The recent results of the theoretical analysis of the model atmospheres of magnetic and chemically peculiar stars are presented. All the calculations are based on the direct opacity sampling technique, and account for the anomalous Zeeman effect and polarized radiation transfer (i.e. full Zeeman treatment). The study includes analyses on the model atmosphere structure, energy distribution, photometric colors, etc., and investigates the role of the magnetic field (its strength and inclination) as well as different chemical compositions (abundance patterns) on the stellar model atmospheres.

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