Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..332..320d&link_type=abstract
The Fate of the Most Massive Stars, ASP Conference Series, Vol. 332, Proceedings of the conference held 23-28 May, 2004 in Grand
Astronomy and Astrophysics
Astronomy
Scientific paper
Massive stars (⪆ 8M&sun;) shape their own environments, due to the combined action of winds, radiation and stellar outbursts. We discuss the nature and evolution of the medium around massive stars, with specific reference to a 35M&sun; star, and show that it is hard to infer the properties of the stellar mass-loss from observations of the circumstellar medium around evolved stars.
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