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Recent Results on Abundance Determinations

Published online by Cambridge University Press:  12 April 2016

Saul J. Adelman
Saul J. Adelman*
Affiliation:
Department of Physics, The Citadel, Charleston, SC 29409USA
*
*Guest Investigator, Dominion Astrophysical Observatory, Hertzberg Institute of Astrophysics, National Research Council of Canada

Abstract

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I review abundance determinations of normal B5-F4 and peculiar stars published since 1984. Several analyses performed with photographic spectrograms indicate interesting stars which should be analyzed with high signal-to-noise data. Studies of stars of known ages which belong to clusters, associations, and moving groups should led to the most direct confrontations with theory. The increase in signal-to-noise ratio provided by electronic detectors with respect to photographic plates should allow accurate analyses of moderating rotating stars. High resolution, high signal-to-noise ratio studies have revealed crucial information about the line profiles of Sirius, Vega, and other A stars. It would aid comparison of analyses if we could agree on a standard set of gf-values and line damping constants. A computer bulletin board would be a useful means to provide and maintain such data as well as model atmosphere codes.

Type
I. General Properties of CP Stars
Information
International Astronomical Union Colloquium , Volume 138: Peculiar versus Normal Phenomena in A-Type and Related Stars , 1993 , pp. 27 - 41
Copyright
Copyright © Astronomical Society of the Pacific 1993

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