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Massive Stars Spectroscopy in the Magellanic Clouds

Published online by Cambridge University Press:  25 May 2016

K. A. Venn
K. A. Venn*
Affiliation:
Macalester College, Department of Physics & Astronomy, 1600 Grand Ave., St. Paul, MN, 55105, USA

Abstract

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Recent results from spectroscopic studies of Magellanic Cloud stars are discussed. Emphasis is placed on how to interpret CNO abundances to examine stellar evolution scenarios. Observed CNO abundances are best explained by the new rotating stellar evolution models (see Langer & Heger, these proceedings). In addition, the Rolleston et al. (these proceedings) abundances for B stars in the Magellanic Bridge are discussed.

Type
Part 3. Massive Stars and 30 Doradus
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 200 - 207
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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