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New Ways to Rotation Rates

Published online by Cambridge University Press:  12 April 2016

R. E. Wilson
R. E. Wilson*
Affiliation:
Department of Astronomy and Space Astronomy Laboratory, 211 SSRB,University of Florida, Gainesville,FL 32611

Abstract

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Progress in determining rotation rates of Algol primary stars from light curves is assessed. Included are elementary ideas on why the new method works, how to carry out solutions, and how and when to apply the constraint on rotational lobe filling. Some comments are made on desirable improvements for measuring rotation from line broadening. A few remarks are made about the problem of identifying likely fast rotating Algols.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 107: Algols , 1989 , pp. 235 - 243
Copyright
Copyright © Kluwer 1989

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