Hostname: page-component-5c6d5d7d68-7tdvq Total loading time: 0 Render date: 2024-08-22T17:19:46.406Z Has data issue: false hasContentIssue false
  • English
  • Français

Population synthesis of binary relativistic stars

Published online by Cambridge University Press:  12 May 2006

V. M. Lipunov
V. M. Lipunov
Affiliation:
Sternberg Astronomical Institute, Moscow State University, Russia 13, Universitetskij pr-t, Moscow, Russia email: [email protected] Present address: Sternberg Astronomical Institute, 13, Universitetskij pr-t, Moscow, Russia.
Rights & Permissions [Opens in a new window]

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.

Population synthesis of binary stars with relativistic component is presented.

Keywords

population synthesisbinary starsrelativistic starshigh energy sources
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S230: Populations of High Energy Sources in Galaxies , August 2005 , pp. 391 - 400
Copyright
2006 International Astronomical Union