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Observational Evidence for Evolutionary Connections Between Wolf-Rayet Stars and Red Supergiants
Published online by Cambridge University Press: 03 August 2017
Extract
The main question in our understanding of the nature of W R stars is: which stars are their progenitors and how do they evolve to reach the WR stage? We have some ideas about progenitor's masses and, by mass luminosity relations, about their brightness when they are 0 stars. But, it is difficult to say anything for their possible Red phase.
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- Session VII. Evolution
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- Copyright © Kluwer 1991