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The colliding wind-formed structures of supernova precursors

Published online by Cambridge University Press:  07 August 2017

O. A. Tsiopa
O. A. Tsiopa*
Affiliation:
Central Astronomical Observatory of the Russian Academy of Sciences, Pulkovo, 196140 St.Petersburg, Russia

Abstract

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The wind interaction processes in supernova precursors can be responsible for the formation of regular structures of the circumstellar matter not only at the distances of 1018 cm (SN1987A), but also at those of less than 1016 cm.

Type
Session VII - Hydrodynamics and high-energy physics of colliding winds
Information
Symposium - International Astronomical Union , Volume 163: Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution , 1995 , pp. 425 - 428
Copyright
Copyright © Kluwer 1995 

References

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