Hostname: page-component-77c89778f8-vsgnj Total loading time: 0 Render date: 2024-07-19T17:23:40.609Z Has data issue: false hasContentIssue false

Solar Type Contact Binaries - The Initial Mass Ratio Distribution Function.

Published online by Cambridge University Press:  14 August 2015

Frans Van 'T Veer*
Affiliation:
Institut d'Astrophysique, Paris

Extract

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.

From a study of the mass ratio function of magnetically active contact binaries it is shown that the great majority of newly formed systems must possess nearly equal components.

Type
IX. Contact Binaries
Copyright
Copyright © Reidel 1980 

References

Huang, S.-S. : 1966, Ann. d'Astrophys. 29, 331 Google Scholar
Okamoto, I. Sato, K. : 1970, Publ. Astr. Soc. Japan 22, 317.Google Scholar
Van 't Veer, F. : 1978, Astron. Astrophys. 70, 91 Google Scholar
Van 't Veer, F. : 1979, Astron. Astrophys.Google Scholar