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CNO abundances in Early Type Be Stars
Published online by Cambridge University Press: 26 May 2016
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.
- Type
- Session 2 Rotation in Relation with Abundances and Magnetic Fields
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- Copyright © Astronomical Society of the Pacific 2004
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