Hostname: page-component-77c89778f8-fv566 Total loading time: 0 Render date: 2024-07-22T06:19:06.234Z Has data issue: false hasContentIssue false
  • English
  • Français

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

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 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

Dopita, A.M., Evans, R., Cohen, M., & Schwarte, R.D. 1984, ApJ, 287, L69 Google Scholar
Niemela, V.S., Ruiz, M.T., & Phillips, M.M. 1985, ApJ, 289, 52 Google Scholar
Polcaro, V.F., & Viotti, R. 1991, A&A, 242, L9 Google Scholar
Tsiopa, O.A. 1990, Astronomicheskj Tsirkular, No. 1554, 23 Google Scholar
Tsiopa, O.A. 1995, in: van der Hucht, K.A. and Williams, P.M. (eds.), Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution (Dordrecht:Kluwer), 425 Google Scholar