INTERACTION OF SUPERNOVA BLAST WAVES WITH WIND-DRIVEN SHELLS: FORMATION OF

Автор(и)

  • V. V. Gvaramadze Abastumani Astrophysical Observatory, Georgian Academy of Sciences, A.Kazbegi ave. 2-a, Tbilisi, 380060, Georgia; Sternberg State Astronomical Institute, Moscow, Russia; Abdus Salam International Centre for Theoretical Physics, Trieste, Italy, Україна

DOI:

https://doi.org/10.18524/1810-4215.1999.12.93025

Ключові слова:

ISM, bubbles, supernova remnants.

Анотація

Most of middle-aged supernova remnants (SNRs) have a distorted and complicated appearance which cannot be explained in the framework of the Sedov-Taylor model. We consider three typical examples of such SNRs (Vela SNR, MSH15-52, G309.2-00.6) and show that their structure could be explained as a result of interaction of a supernova (SN) blast wave with the ambient medium preprocessed by the action of the SN progenitor's wind and ionized emission.

Посилання

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2017-03-16

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