Model atmospheres of magnetic and chemically peculiar stars
- Author(s)
- Sergej Kahn, Denis Victorovich Shulyak
- Abstract
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.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- University of Western Ontario
- Journal
- Contributions of the Astronomical Observatory Skalnaté Pleso
- Volume
- 38
- Pages
- 267-272
- No. of pages
- 6
- ISSN
- 1335-1842
- Publication date
- 2008
- Austrian Fields of Science 2012
- 103003 Astronomy
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/ade01c0f-be36-4aa7-a6ec-10eaf13f434c