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Abstract: The past decade has witnessed impressive progress in our understanding of thephysical properties of massive stars in the Magellanic Clouds, and how theycompare to their cousins in the Galaxy. I summarise new results in this field,including evidence for reduced mass-loss rates and faster stellar rotationalvelocities in the Clouds, and their present-day compositions. I also discussthe stellar temperature scale, emphasizing its dependence on metallicity acrossthe entire upper-part of the Hertzsprung-Russell diagram.



Autor: Christopher J. Evans UKATC, Edinburgh

Fuente: https://arxiv.org/



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