Abstract
The positions of 3218 C stars, 741 S stars and 1140 open clusters have been compared. 59 C stars and 15 S stars have been found to lie in the line of sight to open clusters. This is no more than could be expected from a random distribution of the stars.
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References
Blanco,V.M. 1965, in Galactic Structure, ed. A. Blaauw and M. Schmidt, Univ. Chicago Press, Chicago.
Lyngå,G. 1983, A Catalogue of Open Cluster Data Lund Observatory.
Scalo,J.M., Miller,G.E. 1979, Ap.J. 3233, 596.
Stephenson,C.B. 1973, Publ. Warner Swasey Obsvol.1,no.2
Stephenson,C.B. 1976, Publ. Warner Swasey Obsvol.2,no.2.
Yorka,S.B., Wing,R.F, 1979, Astron.J., 84, 1010.
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© 1985 D. Reidel Publishing Company
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Jϕrgensen, U.G. (1985). Carbon Stars and S Stars Near Open Clusters — a statistical approach . In: Jaschek, M., Keenan, P.C. (eds) Cool Stars with Excesses of Heavy Elements. Astrophysics and Space Science Library, vol 114. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5325-3_25
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DOI: https://doi.org/10.1007/978-94-009-5325-3_25
Publisher Name: Springer, Dordrecht
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