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The Short-Period Non-Contact Binary Systems UU Lyn and GR Tau

Published online by Cambridge University Press:  12 April 2016

A. Yamasaki ,
A. Okazaki  and
M. Kitamura
A. Yamasaki
Affiliation:
Dept. Earth Science and Astronomy, University of Tokyo, Tokyo 153, Japan
A. Okazaki
Affiliation:
Tokyo Astronomical Observatory, University of Tokyo, Tokyo 181, Japan
M. Kitamura
Affiliation:
Tokyo Astronomical Observatory, University of Tokyo, Tokyo 181, Japan

Abstract

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Two binary systems UU Lyn (P = 0d.468) and GR Tau (P = 0d.430) are discussed on the basis of BV photoelectric observations and spectroscopic observations which were made between 1980 and 1981 at the Tokyo Astronomical Observatory. The component stars in both systems are found to be still inside their Roche lobes but very close to them.

Type
Part III: Evolutionary Processes in Close Binary Systems
Information
International Astronomical Union Colloquium , Volume 69: Binary and Multiple Stars as Tracers of Stellar Evolution , 1982 , pp. 345 - 349
Copyright
Copyright © Reidel 1982

References

Geyer, E., Kippenhahn, R. and Strohmeier, W.: 1955, Kleine Veröffentl. Bamberg, No. 11.Google Scholar
Götz, W. and Wenzel, W.: 1962a, Mitt. Veränderliche Sterne, No. 628.Google Scholar
Götz, W. and Wenzel, W.: 1962b, Mitt. Veränderliche Sterne, No. 702.Google Scholar
SAC: 1981, Supplemento ad Annuario Cracoviense, No. 52.Google Scholar
Strohmeier, W., Kippenhahn, R. and Geyer, E.: 1957, Kleine Veröffentl. Bamberg, No. 18.Google Scholar
Strohmeier, W., Knigge, R. and Ott, H.: 1963a, Veröffentl. Bamberg, 5, No. 16.Google Scholar
Strohmeier, W., Knigge, R. and Ott, H.: 1963b, Veröffentl. Bamberg, 5, No. 17.Google Scholar