Hostname: page-component-848d4c4894-ndmmz Total loading time: 0 Render date: 2024-05-05T02:23:52.472Z Has data issue: false hasContentIssue false

The Fate of Binary Systems After the Explosion of SNe 1993J and 1994I

Published online by Cambridge University Press:  25 May 2016

Hitoshi Yamaoka*
Affiliation:
Department of Physics, Faculty of Science, Kyushu University, 4-2-1 Ropponmatsu, Chuo-ku, Fukuoka 810, Japan

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 kinematics of the binary systems to which supernovae(SNe) 1993J and 1994I belonged are studied. The kick velocity caused by supernova(SN) asymmetry will highly influence the fate of the system. The survival rates with assumed kick velocity distribution are discussed.

Type
Stellar Evolution in Star Clusters
Copyright
Copyright © Kluwer 1996 

References

Lyne, A.G., Anderson, B. and Salter, M.J. (1982) MNRAS 201, 503520.Google Scholar
Lyne, A.G. and Lorimer, D.R. (1994) Nat. 369, 127129.Google Scholar
Nomoto, K. et al. (1994) Nat. 371, 227229.Google Scholar
Shigeyama, T. et al. (1994) Ap. J. 420, 341347.Google Scholar
Yamaoka, H., Shigeyama, T. and Nomoto, K. (1992) A. Ap. 267, 433438.Google Scholar