Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-26T04:54:46.086Z Has data issue: false hasContentIssue false

Contact Binaries

Published online by Cambridge University Press:  14 August 2015

J. Hazlehurst*
Affiliation:
Hamburger Sternwarte, Hamburg, West Germany

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.

Observational statements about close and contact binaries are compared with the theoretical consequences of assuming that contact binaries have a common convective envelope. It is concluded that such contact systems cannot be in thermal equilibrium, and that the inefficiency of convective heat transport in the common envelope must be allowed for. Even so, current theory seems to predict about equal numbers of contact and semidetached systems of short period, in conflict with the observations.

Type
Research Article
Copyright
Copyright © Reidel 1976 

References

Aizenman, M. L. and Perdang, J.: 1971, Astron. Astrophys. 12, 232.Google Scholar
Aizenman, M. L. and Perdang, J.: 1972, Astron. Astrophys. 19, 315.Google Scholar
Hazlehurst, J. and Meyer-Hofmeister, E.: 1973, Astron. Astrophys. 24, 379.Google Scholar
Hazlehurst, J.: 1974, Astron. Astrophys. 36, 49.Google Scholar
Lucy, L. B.: 1968, Astrophys. J. 151, 1123.Google Scholar
Lucy, L. B.: 1975, submitted to Astrophys. J. Google Scholar
Rucinski, S. M.: 1973, Acta Astron. 23, 79.Google Scholar
Rucinski, S. M.: 1974, Acta Astron. 24, 119.Google Scholar
Tapia, S. and Whelan, J. A. J.: 1975, Astrophys. J. 200, 98.Google Scholar