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Quantitative Analysis of O-Type Stars Properties, at Low Metallicity
Published online by Cambridge University Press: 26 May 2016
Abstract
We have investigated the properties of main-sequence O-type stars in the SMC. Mass-loss rates, luminosities and Teff are much smaller for these stars than for Galactic ones, resulting in a steeper wind-momentum relation.
- Type
- Part 1. Atmospheres of Massive Stars
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- Copyright © Astronomical Society of the Pacific 2003