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Blue Clusters, Populous Clusters, and Globulars

Published online by Cambridge University Press:  04 August 2017

Paul W. Hodge
Paul W. Hodge*
Affiliation:
Astronomy Department, University of Washington, Seattle, WA

Abstract

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The introduction of new photometric techniques for faint objects has tremendously increased our understanding of the MC clusters, especially at the old end of the age spectrum. Many of the well-studied clusters of the past have gone through several transformations, starting as true globulars in 1960, becoming intermediate-age objects in the 1970's, but now returning to the true globular classification in the 1980's. LW 868 is an example of a cluster with such a history. Better photometric accuracy is also greatly improving our understanding of younger clusters, allowing detailed comparisons with theoretical evolutionary models, and a more reliable determination of the age-abundance relationship. The dynamical history of MC clusters can also be examined from the new data. The cluster formation rate, as well as the destruction rate, can be reconstructed from modern, deep cluster surveys.

Type
Magellanic Cloud Clusters
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 7 - 12
Copyright
Copyright © Reidel 1984 

References

Aaronson, M., Olszewski, E. and Schommer, R.: 1983, in preparation.Google Scholar
Andersen, J., Blecha, A., and Walker, M.F.: 1984, this volume, p. 41.Google Scholar
Becker, S. A. and Mathews, G. J.: 1983, Astrophys. J. 270, 155.Google Scholar
Böhm-Vitense, E., Hodge, P. W., and Proffitt, C.: 1983a, preprint.Google Scholar
Böhm-Vitense, E., Hodge, P. W., Nemec, J. and Proffitt, C.: 1983b, preprint.Google Scholar
Brück, M.: 1975, Mon. Not. Royal Astron. Soc. 173, 327.Google Scholar
Cassatella, A. and Geyer, E. H.: 1983, Proc. Third Europ. IUE Conf., 523.Google Scholar
Cohen, J. G.: 1982, Ap. J. 258, 143.Google Scholar
Cowley, A. P. and Hartwick, F. D. A.: 1981, Astron. J. 86, 667.Google Scholar
Cowley, A. P. and Hartwick, F. D. A.: 1982, Astrophys. J. 259, 89.Google Scholar
de Boer, K. S.: 1984, this volume, p. 53.Google Scholar
Feast, M. W.: 1972, Mon. Not. Royal Astron. Soc. 159, 113.Google Scholar
Flower, P. J.: 1982a, Publ. Astron. Soc. Pacific 94, 122.CrossRefGoogle Scholar
Flower, P. J.: 1982b, Publ. Astron. Soc. Pacific 94, 894.Google Scholar
Flower, P.: 1983, preprint.Google Scholar
Flower, P., Geisler, D., Hodge, P., Olszewski, E. and Schommer, R.: 1983, Astrophys. J., in press.Google Scholar
Freeman, K. and Gascoigne, S. C. B.: 1977, Proc. Astron. Soc. Australia 3, 136.Google Scholar
Freeman, K., Illingworth, G. and Oemler, G.: 1983, preprint.Google Scholar
Frenk, C. S. and Fall, S. M.: 1982, Mon. Not. Royal Astron. Soc. 199, 565.Google Scholar
Gascoigne, S. C. B.: 1966, Mon Not. Royal Astron. Soc. 134, 59.Google Scholar
Geisler, D. and Hodge, P. W.: 1980, Astrophys. J. 242, 66.CrossRefGoogle Scholar
Geyer, E. H., Hopp, U., and Nelles, B.: 1983, preprint.Google Scholar
Graham, J. and Nemec, J.: 1984, this volume, p. 37.Google Scholar
Hesser, J., Nemec, J., Stryker, L. and McClure, R.: 1983, preprint.Google Scholar
Hodge, P. W.: 1983a, Astrophys. J. 264, 470.Google Scholar
Hodge, P. W.: 1983b, paper in preparation.Google Scholar
Hodge, P. W. and Lee, S.-O.: 1983, Astrophys. J., in press.Google Scholar
Hodge, P. W. and Morris, V.: 1983, preprint.Google Scholar
Hodge, P. W. and Schommer, R.: 1983, preprint.Google Scholar
Janes, K. and Carney, B.: 1983, preprint.Google Scholar
Kinman, T. D., Stryker, L. L., and Hesser, J. E.: 1983, preprint.Google Scholar
Kontizas, M.: 1980, Astr. Ap. Suppl. 40, 151.Google Scholar
Kontizas, M.: 1983, preprint.Google Scholar
Kontizas, E., Dialetis, D., Prokakis, Th., and Kontizas, M.: 1983, preprint Google Scholar
Mould, J. and Da Costa, G.: 1983, preprint.Google Scholar
Nemec, J.: 1983, Ph.D. dissertation, University of Washington.Google Scholar
Olszewski, E.: 1982, Ph.D. dissertation, University of Washington.Google Scholar
Penny, A. J.: 1975, Mon. Not. Royal Astron. Soc. 172, p. 65 Google Scholar
Rich, R. M., Mould, J. and Da Costa, G.: 1984, this volume, p. 45.Google Scholar
Robertson, J. W.: 1974, Astron. Astrophys. Suppl. 15, 261.Google Scholar
Stryker, L., Butcher, H. and Jewell, J.: 1981, in IAU Colloq. No. 68 (Schenectady, L. Davis Press), p. 267.Google Scholar
van Duine, D.: 1983, preprint.Google Scholar
Walker, M. F.: 1979, Mon. Not. Royal Astron. Soc. 188, 735.Google Scholar
Westerlund, B.: 1961, Ann. Uppsala Astron. Obs. 5, No. 1.Google Scholar
Wielen, R.: 1971, Astron. Astrophys. 13, 309.Google Scholar