CNO abundances in Early Type Be Stars
- 1 January 2004
- journal article
- Published by Cambridge University Press (CUP) in Symposium - International Astronomical Union
- Vol. 215, 222-223
- https://doi.org/10.1017/s0074180900195592
Abstract
High dispersion spectra in the visible range were obtained for field Be Stars in both hemispheres. As Be Stars form a class of Main Sequence fast rotators, we are intended to test how their chemical composition can be affected by rotation.Keywords
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