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Shells around Hot Stars

Published online by Cambridge University Press:  25 April 2016

T.A. Lozinskaya*
Affiliation:
Sternberg Astronomical Insititute, Moscow

Abstract

The influence of the progenitor’s stellar wind on the supernova event, and subsequent development of a remnant are discussed. Various morphological differences between SN remnants and the implications for previous wind activity are described. A detailed look at the effects in the ring nebula NGC 6888 is presented.

Type
Research Article
Copyright
Copyright © Astronomical Society of Australia 1988

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