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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

Adelman, S.J.: 1984, Astron. Astrophys. 58, 585 Google Scholar
Adelman, S.J.: 1985, Astron. Astrophys. Suppl., in pressGoogle Scholar
Hofflelt, D.: 1982, The Bright Star Catalogue, 4th edition (Yale University Observatory: New Haven, CT)Google Scholar
Lane, M.C., Lester, J.B.: 1980, Astrophys. J. 238, 210 Google Scholar
Kurucz, R.L.: 1979, Astrophys. J. Suppl. Ser. 40, 1 Google Scholar
Moore, C.E.: 1945, A Multiplet Table of Astrophysical Interest (Princeton University Observatory: Princeton, NJ)Google Scholar
Reader, J., Corliss, C.H.: 1980, NSRDS-NBS 68, part I (US Government Printing Office: Washington, DC)Google Scholar