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Can We Check by High-Dispersion Analyses Stars Belonging to Eggen's Moving Groups?

Published online by Cambridge University Press:  14 August 2015

L. E. Pasinetti*
Affiliation:
Milano-Merate Observatory, Italy

Abstract

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We describe the results of analysis of the giant star HD 6497, which belongs to the Arcturus group.

Type
Part IV/Abundance Effects in Spectral Classification
Copyright
Copyright © Reidel 1976 

References

Cayrel de Strobel, G.: 1966, Ann. Astrophys. 29, 413.Google Scholar
Cayrel de Strobel, G. and Pasinetti, L. E.: 1975, Astron. Astrophys. 43, 127.Google Scholar
Eggen, O. J.: 1974, Publ. Astron. Soc. Pacific 86, 162.Google Scholar
Foy, R.: 1971, Astron. Astrophys. 11, 89.Google Scholar
Grenon, M.: 1972, private communication.Google Scholar
Hansen, L. and Kjaergaard, P.: 1971, Astron. Astrophys. 15, 123.Google Scholar
Mäckle, R., Holweger, H., Griffin, R. and Griffin, R.: 1975, Astron. Astrophys. 38, 239.Google Scholar
Williams, P. M.: 1971, Monthly Notices Roy. Astron. Soc. 153, 171.Google Scholar