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Chemically Peculiar Stars in Clusters: Upper and Lower Age Limits of CP Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
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The evolutionary state of CP Stars is defined using members of open clusters. It is confirmed that all CP stars belong to the main sequence, if the case of Horizontal-Branch Stars is omitted. The frequency of CP Stars as a function of age has been reconsidered: it is found constant for the CP2 stars, but significantly increasing with age for the CP1 (Am) stars.
- Type
- VII. Photometric Variability and Evolutionary Status
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 1993
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