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The Metallic-Lined Star 32 Aquarii

Published online by Cambridge University Press:  12 April 2016

Dursun Kocer ,
Cetin Bolcal  and
Saul J. Adelman
Dursun Kocer
Affiliation:
Kandilli Observatory of Bogazici UniversityCengelkoy, Istanbul, Turkey
Cetin Bolcal
Affiliation:
Kandilli Observatory of Bogazici UniversityCengelkoy, Istanbul, Turkey
Saul J. Adelman
Affiliation:
Code 681, Laboratory for Astronomy and Solar Physics NASA Goddard Space Flight Center Greenbelt, MD 20771, United States of America

Abstract

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Prelimary results from an optical region study of the metallic-lined star 32 Aquarii indicate Teff = 7600 K, log g = 3.10, ξ = 4.6 km s−1, and an iron abundance about one-half solar.

Type
Section IV - Non-Magnetic CP and Related Stars
Information
International Astronomical Union Colloquium , Volume 90: Upper Main Sequence Stars with Anomalous Abundances , 1986 , pp. 455 - 457
Copyright
Copyright © Reidel 1986

References

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