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Shells around Hot Stars
Published online by Cambridge University Press: 25 April 2016
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.
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- Research Article
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- Copyright © Astronomical Society of Australia 1988
References
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