Hostname: page-component-cd9895bd7-q99xh Total loading time: 0 Render date: 2024-12-26T15:26:51.058Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Adelman, S. J. 1984, Monthly Notices Roy. Astron. Soc. 206, 637.CrossRefGoogle Scholar
Adelman, S. J. 1985, in preparation.Google Scholar
Adelman, S. J., Young, J. M. and Baldwin, H. E. 1984, Monthly Notices Roy. Astron. Soc. 206, 649.CrossRefGoogle Scholar
Baschek, G. and Reimers, D. 1969, Astron. Astrophys. 2, 240.Google Scholar
Blackwell, D. E., Petford, A. D., Shallis, M. J. and Simmons, G. J. 1982, Monthly Notices Roy. Astron. Soc. 199, 43.CrossRefGoogle Scholar
Hayes, D. S. and Latham, D. W. 1975, Astrophys. J. 197, 593.CrossRefGoogle Scholar
Kurcuz, R. L. 1979, Astrophys. J. Suppl. 40, 1.CrossRefGoogle Scholar