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Supernovae in Massive Interacting Binaries

Published online by Cambridge University Press:  07 August 2017

P. C. Joss ,
J. J. L. Hsu ,
Ph. Podsiadlowski  and
R. R. Ross
P. C. Joss
Affiliation:
1M. I. T, Cambridge, MA 02139, U.S.A.
J. J. L. Hsu
Affiliation:
1M. I. T, Cambridge, MA 02139, U.S.A. 2University of California, Berkeley, CA 94720, U.S.A.
Ph. Podsiadlowski
Affiliation:
3Institute of Astronomy, Cambridge CB3 0HA, U.K.
R. R. Ross
Affiliation:
4College of the Holy Cross, Worcester, MA 01610, U.S.A.

Abstract

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We here report the results of a systematic investigation of how binary interaction affects the presupernova evolution of massive stars and the resulting supernova explosions. We summarize the various types of binary interaction and the evolutionary scenarios in which they are realized. We also present the results of a series of hydrodynamical calculations which model the supernova explosion for various progenitor types and discuss their observable characteristics.

Type
Oral and Contributed Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 523 - 526
Copyright
Copyright © Kluwer 1992 

References

Hsu, J. J. L., Ross, R. R., Joss, P. C., and Podsiadlowski, Ph. (1992), in preparation.Google Scholar
Podsiadlowski, Ph., Joss, P. C., Hsu, J. J. L. (1992), in press.Google Scholar