Mass-loss predictions and stellar masses of early-type stars
Abstract
Description
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.
2 pages; in: A Massive Star Odyssey, from Main Sequence to Supernova
2 pages; in: A Massive Star Odyssey, from Main Sequence to Supernova