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Cool Carbon Stars in Open Clusters

Published online by Cambridge University Press:  14 August 2015

A. Alksnis  and
Z. Alksne
A. Alksnis
Affiliation:
Radioastrophysical Observatory, Latvian Academy of Sciences, Latvia, U.S.S.R.
Z. Alksne
Affiliation:
Radioastrophysical Observatory, Latvian Academy of Sciences, Latvia, U.S.S.R.

Abstract

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By combining lists of carbon stars with the catalogue of open clusters (Alter et al., 1970), a list of variable carbon stars, being probable members of clusters is given. The number of stars is too small to derive reliable statistics on cluster membership. Too few radial velocities are yet available. Photometric criteria are still too inaccurately known.

Type
Part 2 / R Coronae Borealis Stars
Information
Symposium - International Astronomical Union , Volume 67: Variable Stars and Stellar Evolution , 1975 , pp. 173
Copyright
Copyright © Reidel 1975 

References

Alter, G., Ruprecht, J., and Vanýsek, V.: 1970, Catalogue of Star Clusters, 2nd ed., Budapest.Google Scholar
Baumert, J. H.: 1974, Astrophys. J. 190, 85.Google Scholar