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Shells around Hot Stars

Published online by Cambridge University Press:  25 April 2016

T.A. Lozinskaya
T.A. Lozinskaya*
Affiliation:
Sternberg Astronomical Insititute, Moscow
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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
Information
Publications of the Astronomical Society of Australia , Volume 7 , Issue 4 , 1988 , pp. 535 - 539
Copyright
Copyright © Astronomical Society of Australia 1988

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