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Element abundances from B stars in the Magellanic Clouds
Published online by Cambridge University Press: 19 July 2016
Abstract
High resolution spectrograms of B stars in the blue globular cluster NGC 2004, located in the Large Magellanic Cloud (LMC), have been used to derive chemical abundances, differentially with respect to a galactic comparison star.
- Type
- Stellar Evolution
- Information
- Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 388 - 389
- Copyright
- Copyright © Kluwer 1991
References
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