Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-19T11:36:52.230Z Has data issue: false hasContentIssue false
  • English
  • Français

The Integrated Spectra of Star Clusters and the History of the Magellanic Clouds

Published online by Cambridge University Press:  04 August 2017

Leonard Searle
Leonard Searle*
Affiliation:
Mount Wilson and Las Campanas Observatories of the Carnegie Institution of Washington

Abstract

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.

This paper reviews the attempts that have been made to derive the ages and compositions of star clusters from studies of their integrated light. It discusses what can be learned by such methods regarding the history of the Magellanic Clouds. Finally, it reviews what is known about the age-spread and abundance-range in the cluster-systems of other galaxies and considers the history of the Magellanic Clouds in this context.

Type
Magellanic Cloud Clusters
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 13 - 23
Copyright
Copyright © Reidel 1984 

References

Aaronson, M., Cohen, J.G., Mould, J., and Malkan, M.: 1978, Astrophys. J. 223, 824.CrossRefGoogle Scholar
Arp, H.C., and Cuffey, J.: 1962, Astrophys. J. 138, 356.Google Scholar
Barbaro, G., and Bertelli, G.: 1977, Astron. Astrophys 54, 243.Google Scholar
Christian, C.A., and Schommer, R.A.: 1982, Astrophys. J. Suppl. 49, 353.Google Scholar
Cohen, J.G.: 1982, Astrophys. J. 258, 143.Google Scholar
Danziger, I.J.: 1973, Astrophys. J. 181, 641.CrossRefGoogle Scholar
Frenk, C.S., and Fall, S.M.: 1982, M.N.R.A.S. 199, 565.Google Scholar
Frogel, J.A., Persson, S.E., and Cohen, J.G.: 1980, Astrophys. J. 240, 785.Google Scholar
Gelfand, A.E.: 1969, Thesis, Stanford University, University Microfilms, Ann Arbor, Michigan.Google Scholar
Hardy, E.: 1981, Astron. J. 86, 217.Google Scholar
Hiltner, W.: 1960, Astrophys. J. 131, 163.Google Scholar
Hodge, P.W.: 1983, Astrophys. J. 264, 470.CrossRefGoogle Scholar
Larson, R.B., and Tinsley, B.M.: 1978, Astrophys. J. 219, 46.CrossRefGoogle Scholar
Pagel, B.E.J., and Edmunds, M.G.: 1981, Ann. Rev. Astron. Astrophys. 19, 77.CrossRefGoogle Scholar
Persson, S.E., Aaronson, M., Cohen, J.G., Frogel, J.A., and Matthews, K.: 1983, Astrophys. J. 266, 105.CrossRefGoogle Scholar
Rabin, D.: 1982, Astrophys. J. 261, 85.CrossRefGoogle Scholar
Sandage, A.R.: 1963, Astrophys. J. 138, 863.CrossRefGoogle Scholar
Sandage, A.R., and Carlson, G.: 1983, Astrophys. J. (Letters) 267, L25.Google Scholar
Searle, L., and Sargent, W.L.W.: 1972, Astrophys. J. 173, 25.CrossRefGoogle Scholar
Searle, L., Sargent, W.L.W., and Bagnuolo, W.G.: 1973, Astrophys. J. 179, 427.CrossRefGoogle Scholar
Searle, L., Wilkinson, A., and Bagnuolo, W.G.: 1980, Astrophys J. 239, 803.CrossRefGoogle Scholar
Shectman, S.A.: 1981, Ann. Report of the Director, Mount Wilson and Las Campanas Observatories, 1980–81, p. 586.Google Scholar
van den Bergh, S.: 1969, Astrophys. J. Suppl. 19, 145.CrossRefGoogle Scholar
Vetesnik, M.: 1962, Bull Ast. Inst. Czechoslovakia 13, 180.Google Scholar
Webster, B.L., and Smith, M.G.: 1983, M.N.R.A.S. 204, 743.CrossRefGoogle Scholar
Zinn, R.J.: 1980, Astrophys. J. Suppl. 42, 19.Google Scholar