Facebook Instagram Twitter RSS Feed PodBean Back to top on side

Model atmospheres of magnetic and chemically peculiar stars

In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2
S.a. Khan - D.v. Shulyak

Details:

Year, pages: 2008, 267 - 272
Keywords:
stars: chemically peculiar, stars: atmospheres, stars: magnetic fields, stars: abundances
About article:
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.
How to cite:
ISO 690:
Khan, S., Shulyak, D. 2008. Model atmospheres of magnetic and chemically peculiar stars. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no.2, pp. 267-272. 1335-1842.

APA:
Khan, S., Shulyak, D. (2008). Model atmospheres of magnetic and chemically peculiar stars. Contributions of the Astronomical Observatory Skalnaté Pleso, 38(2), 267-272. 1335-1842.