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Abundances of Be Stars in Very Young Open Clusters
Published online by Cambridge University Press: 12 April 2016
Abstract
We present here standard uvbyβ CCD photometry for five open clusters of the Galaxy in order to determine abundances of Be stars, as a function of age.
- Type
- 1. Overview
- Information
- International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 59 - 62
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
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