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Elemental Abundances of Normal Sharp-Lined B and A Stars from Optical Region Analyses

Published online by Cambridge University Press:  04 August 2017

Saul J. Adelman
Saul J. Adelman*
Affiliation:
Department of Physics, The Citadel

Abstract

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Optical-region elemental-abundance analyses were performed for ten sharp-lined main sequence B and A stars. The derived abundances are generally in good agreement with those of the Sun. Multiple high dispersion spectrograms, fully line-blanketed solar composition model atmospheres, optical spectrophotometry, and the most accurate gf values were employed. This study provides initial parameters for studies of these stars in the ultraviolet and a consistent set of values for comparison with abundances of more exotic stars.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 111: Calibration of Fundamental Stellar Quantities , 1985 , pp. 423 - 426
Copyright
Copyright © Reidel 1985 

References

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