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Helium-Rich Stellar Atmosphere Models for B Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
The hydrogen and helium line equivalent widths from stellar atmosphere models for early B stars are presented. The models, which range in helium number fraction from 0.10 to 0.85, result from the non-LTE statistical equilibrium code of Mihalas.
- Type
- VI Intermediate Helium Stars
- Information
- International Astronomical Union Colloquium , Volume 87: Hydrogen Deficient Stars and Related Objects , 1985 , pp. 297 - 300
- Copyright
- Copyright © Reidel 1986
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