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Abstract: We review recent advances in our understanding of massive stars through theanalysis of their spectra. Improvements in model atmospheres and analysismethods are briefly discussed. Results obtained for stars in the Local Groupare compared and the present status of different open questions, like thetemperature scale of OB stars, the Wind Momentum-Luminosity Relation or thestellar rotation, is outlined.



Autor: A. Herrero

Fuente: https://arxiv.org/







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