Hostname: page-component-76fb5796d-wq484 Total loading time: 0 Render date: 2024-04-29T06:07:14.464Z Has data issue: false hasContentIssue false
  • English
  • Français

Extended Surveys of MC Star Clusters

Published online by Cambridge University Press:  26 July 2016

M. Kontizas  and
E. Kontizas
M. Kontizas
Affiliation:
Section of Astrophysics, Astronomy and Mechanics, Department of Physics, University of Athens, Greece
E. Kontizas
Affiliation:
Astronomical Institute, National Observatory of Athens, P.O. Box 20 048, Thission, Athens, Gr-118 10, Greece

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.

The location of the LMC clusters, their age distribution and dynamical parameters have shown that two star cluster systems exist in this galaxy: 1) one extended system, elliptical in shape, which contains all intermediate and old star clusters and 2) another system, again elliptical, but smaller in diameter, superimposed on the other and inclined by about 50 degrees from the latter. It contains the most massive, very young globular clusters which are still at their early phases of dynamical evolution. The existence of very rich stellar associations, binary star clusters and very elliptical ones located in this system, indicates that massive star clusters have formed very recently and are still under formation.

Type
Part Ten: The Magellanic Clouds
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 497 - 501
Copyright
Copyright © Kluwer 1994 

References

Argyropoulos, S., Kontizas, E., Kontizas, M. and Dapergolas, A., 1993. In preparation.Google Scholar
Chrysovergis, M., Kontizas, M. and Kontizas, E., 1989. Astron. & Astrophys. Suppl., 77, 357.Google Scholar
Chrysovergis, M., 1991. PhD Thesis, Athens University.Google Scholar
Freeman, K.C., 1970. Astrophys. J., 160, 811.Google Scholar
Freeman, K.C., Illingworth, G. and Oemler, A., 1983. Astron. J., 272, 488.CrossRefGoogle Scholar
Geyer, E.H. and Hopp, U., 1980. Astroph. & Sp. Sci. 69, 495.Google Scholar
Hodge, P., 1988. Publ. Astron. Soc. Pacific, 100, 1051.CrossRefGoogle Scholar
Kontizas, E., Kontizas, M. and Xiradaki, E., 1987a. Astron. & Astrophys. Suppl., 71, 575.Google Scholar
Kontizas, E., Metaxa, M. and Kontizas, M., 1988. Astron. J., 96, 1625.Google Scholar
Kontizas, E., Kontizas, M., Sedmak, G. and Smareglia, R., 1989. Astron. J., 98, 590.Google Scholar
Kontizas, M., Morgan, D.H., Hadzidimitriou, D. and Kontizas, E., 1990. Astron. & Astrophys. Suppl., 84, 257.Google Scholar
Kontizas, M. and Kontizas, E., 1991. In ‘Formation and Evolution of Star Clusters’, Astronomical Society of the Pacific Conference Series, ed. Janes, K. A., p. 407.Google Scholar
Schommer, R.A., 1991. In: ‘The Magellanic Clouds’, Proc. IAU Symp. 148, eds. Haynes, R., Milne, D., p. 132.Google Scholar
Zinn, R., 1990. Roy Astr. Soc. Con., Vol. 84, 89.Google Scholar