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2006•Astronomy and AstrophysicsOpen access

Stellar model atmospheres with magnetic line blanketing

S. Khan, D. Shulyak

Open full text 15 citations

Abstract

Context.We introduced the technique of model atmosphere calculation with polarized radiative transfer and magnetic line blanketing. However, the calculation of model atmospheres with realistic magnetic field configurations (field strength and angle defined relative to the atmosphere plane) has not been previously attempted.

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What this paper is about

Context.We introduced the technique of model atmosphere calculation with polarized radiative transfer and magnetic line blanketing. However, the calculation of model atmospheres with realistic magnetic field configurations (field strength and angle defined relative to the atmosphere plane) has not been previously attempted.

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Available abstract

Context.We introduced the technique of model atmosphere calculation with polarized radiative transfer and magnetic line blanketing. However, the calculation of model atmospheres with realistic magnetic field configurations (field strength and angle defined relative to the atmosphere plane) has not been previously attempted.

Key concepts: Blanketing, Balmer series, Physics, Magnetic field, Zeeman effect, Astrophysics, Stellar atmosphere, Context (archaeology)

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