Article contents
Massive Stars Spectroscopy in the Magellanic Clouds
Published online by Cambridge University Press: 25 May 2016
Abstract
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
References
- 1
- Cited by