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Mass-loss predictions and stellar masses of early-type stars
Published online by Cambridge University Press: 26 May 2016
Abstract
We show that the stellar masses implied by our predictions of the wind properties of massive stars are in agreement with masses derived from evolution theory and from direct measurements using spectroscopic binaries, contrary to previous attempts to derive masses from wind theory.
- Type
- Part 1. Atmospheres of Massive Stars
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- Copyright © Astronomical Society of the Pacific 2003
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