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A Spectroscopic Study of Epsilon Aurigae*

Published online by Cambridge University Press:  12 April 2016

Mamoru Saitō ,
Shusaku Kawabata ,
Keiich Saijo  and
Hideo Sato
Mamoru Saitō
Affiliation:
Department of Astronomy, Kyoto University, Kyoto, Japan
Shusaku Kawabata
Affiliation:
Kyoto Gakuen University, Kameoka, Kyoto, Japan
Keiich Saijo
Affiliation:
National Science Museum, Ueno Park, Tokyo, Japan
Hideo Sato
Affiliation:
Tokyo Astronomical Observatory, Mitaka, Tokyo, Japan

Abstract

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Epsilon Aurigae has been observed during ingress and totality between 1982 and 1983 at Okayama. Analyses of profiles of Ha line and of radial velocities of neutral hydrogen and metals show that the secondary component consists of at least three parts in structure.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 80: Double Stars, Physical Properties and Generic Relations , 1984 , pp. 269 - 272
Copyright
Copyright © Reidel 1984

Footnotes

*

Paper presented at the Lembang-Bamberg IAU Colloquium No. 80 on ‘Double Stars: Physical Properties and Generic Relations', held at Bandung, Indonesia, 3-7 June, 1983.

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