Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-26T03:53:48.224Z Has data issue: false hasContentIssue false
  • English
  • Français

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

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.

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