Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-19T04:54:16.054Z Has data issue: false hasContentIssue false
  • English
  • Français

Stellar Evolution and Mass Transfer in Binaries

Published online by Cambridge University Press:  12 April 2016

A.A. Bojarchuk ,
V.M. Chechetkin ,
O.A. Kuznetzov  and
Yu.P. Popov
A.A. Bojarchuk
Affiliation:
Institute of Astronomy, Moscow, Russia.
V.M. Chechetkin
Affiliation:
Keldysh Institute of Applied Mathematics, Moscow, Russia.
O.A. Kuznetzov
Affiliation:
Keldysh Institute of Applied Mathematics, Moscow, Russia.
Yu.P. Popov
Affiliation:
Keldysh Institute of Applied Mathematics, Moscow, Russia.

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.

The problem of angular momentum loss in binaries and its influence on stellar evolution is considered. The results of 2D hydrodynamics computer simulation of mass transfer is presented.

Type
XI. Supplement
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 807 - 809
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Chechetkin., V.M., Gerstein, S.S., Imshennik, V.S., Ivanova, L.N., Khlopov, M.Yu. 1980, Astrophys. and Space Sci., 67, p.61.CrossRefGoogle Scholar
Iben, I. Jr., and Tutukov, A.V. 1984, Ap.J.Suppl, 54, p.335.Google Scholar
Masevich, A.G. and Tutukov, A.V., 1988, Evolution of Stars - Theory and observation, Moscow, Nauka.Google Scholar