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The Mass Loss and Pulsation Activity in Supernova Progenitors

Published online by Cambridge University Press:  12 April 2016

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-formed regular structures revealed in early supernova (SN) spectra can be a result of the radial pulsation of the precursor.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 397 - 398
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

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