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An Abundance Analysis of the Silicon CP Star HD 43819

Published online by Cambridge University Press:  12 April 2016

Zulema Lopez-Garcia  and
Saul J. Adelman
Zulema Lopez-Garcia*
Affiliation:
Observatorio Astronomico “Felix Aguilar”, Universidad Nacional de San Juan, San Juan, Argentina
Saul J. Adelman
Affiliation:
Department of Physics, The Citadel, Charleston, SC 29409USA
*
(1)Member of the Can-era del Investigador Cientlfico, CONICET, Argentina

Abstract

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A fine analysis performed using four 4.3 Å/mm IIaO Mt. Wilson Observatory spectrograms shows that HD 43819 has abundance anomalies similar to those of other Silicon stars, namely it is helium, carbon, magnesium, and sulfur poor while being silicon, titanium, chromium, manganese, iron, strontium, zirconium, and rare earth rich.

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. 149 - 153
Copyright
Copyright © Astronomical Society of the Pacific 1993

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