Hostname: page-component-7bb8b95d7b-lvwk9 Total loading time: 0 Render date: 2024-10-01T08:11:59.812Z Has data issue: false hasContentIssue false
  • English
  • Français

Some Color-Magnitude Diagrams and Abundances in the Magellanic Clouds

Published online by Cambridge University Press:  14 August 2015

Eduardo Hardy ,
Jorge Melnick  and
Claude Reheault
Eduardo Hardy
Affiliation:
Dept. de Physique, Université Laval, Québec, Canada European Southern Observatory, Geneva
Jorge Melnick
Affiliation:
European Southern Observatory, Geneva
Claude Reheault
Affiliation:
Dept. de Physique, Université Laval, Québec, Canada

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Some C-M diagrams and photometric abundances are presented of clusters and their adjoining fields in areas of the Clouds, in an attempt to derive properties which would allow a comparison with regions in the Galaxy.

Type
August 29 Open And Globular Clusters
Information
Symposium - International Astronomical Union , Volume 85: Star Clusters , 1980 , pp. 343 - 345
Copyright
Copyright © Reidel 1980 

References

Arp, H., and Cuffey, J.: 1962, Astrophys. J. 136, 51.Google Scholar
Canterna, R.: 1976, Astrophys. J. 81, 228.Google Scholar
Gascoigne, S.C.B.: 1976, Astrophys. J. 209, L25.Google Scholar
Harris, H.C., and Canterna, R.: 1977, Astron. J. 82, 798.Google Scholar
Janes, K.A.: 1979, Astrophys. J. Supp. 39, 135.Google Scholar
Walker, M.F.: 1970, Astrophys. J. 161, 835.Google Scholar
Walker, M.F.: 1971, Astrophys. J. 167, 1.Google Scholar