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The Environs of Supernova Precursors

Published online by Cambridge University Press:  07 August 2017

O.A. Tsiopa
O.A. Tsiopa*
Affiliation:
Pulkovo Observatory, St. Petersbourg, 196140 Russia

Extract

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A high activity of a precursor during the last years of its existence can be connected with a close binary system orbit changing.

Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 409
Copyright
Copyright © Kluwer 1993 

References

Iben, I. Jr. and Tutukov, A.U. (1984). “Supernovae of type I as end products of the evolution of binaries with components of moderate initial mass”, Astrophys. J. Supplement, 54, 335–372 Google Scholar
Polcaro, V.F. and Viotti, R. (1991), “H absorbtion in the type–Ia supernova 1990 M during its early phases”, Astronomy and Astrophysics, 242, L9–L11 Google Scholar
Tsiopa, O.A. (1992), “The non–symmetric structure of the stellar wind of the supernova precursor”, in “Bipolar outflows and stellar jets”.Google Scholar