Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-28T22:29:44.147Z Has data issue: false hasContentIssue false

Barrel-like Supernova Remnants

Published online by Cambridge University Press:  25 April 2016

G. S. Bisnovatyi-Kogan
Affiliation:
Space Research Institute of the USSR Academy of Sciences, Moscow, USSR
T. A. Lozinskaya
Affiliation:
Stenberg State Astronomical Institute, Moscow, USSR
S. A. Silich
Affiliation:
Main Astronomical Observatory of the Ukrainian Academy of Sciences, Kiev, USSR

Abstract

The origin of cylindrically symmetric supernova remnants (SNR) is discussed. The results of numerical simulations of the two best examples of barrel-like SNRs, SN 1006 and G296.5+10.0, are presented.

Type
Galactic and Stellar
Copyright
Copyright © Astronomical Society of Australia 1991

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Bisnovatyi-Kogan, G. S. and Blinnicov, S. I., 1982, Astron. ZH, 59, 876.Google Scholar
Bisnovatyi-Kogan, G. S., Blinnicov, S. I. and Silich, S. A., 1989, Astrophys. Space Sci. 154, 229.CrossRefGoogle Scholar
Kesteven, M. J. and Caswell, J. L., 1987, Astron. Astrophys., 183, 118.Google Scholar
Roger, R. S., Milne, D. K., Kesteven, M. J., Wellington, K. J., Haynes, R.F., 1988, Astrophys. J., 332, 940.CrossRefGoogle Scholar