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Star Formation of Star Clusters in the SMC and their Adjoining Fields

Published online by Cambridge University Press:  04 August 2017

M. Kontizas  and
E. Kontizas
M. Kontizas
Affiliation:
* University of Athens
E. Kontizas
Affiliation:
** National Observatory

Extract

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Photometric and recent spectroscopic studies of the SMC have shown that the differences observed in the SMC clusters and those of our Galaxy could be attibuted to differences in metallicity, star formation rate and/or the Initial Mass Function (IMF) (Humphries, 1983). The studied clusters NGC152 and KRON3 are located at the west side of the bar of the SMC and their adjoining fields represent the halo population of this galaxy.

Type
Poster Papers - Sessions 1 and 2
Information
Symposium - International Astronomical Union , Volume 116: Luminous Stars and Associations in Galaxies , 1986 , pp. 101 - 102
Copyright
Copyright © Reidel 1986 

References

Humphries, R. M.: 1983, Ap. J., 265, 176.CrossRefGoogle Scholar
Kontizas, M., Kontizas, E. and Stewart, N.: 1984, IAU, Symp No 105, p. 121.CrossRefGoogle Scholar
Kontizas, E., Dapergolas, A. and Kontizas, M.: 1985, submitted.Google Scholar
Miller, G.E., and Scalo, J. M.: 1982, Ap. J. 263, 259.CrossRefGoogle Scholar
Stryker, L. L.: 1984, IAU Symp. No 108, p. 79.Google Scholar
Stewart, N.: 1980, Edinburgh University.Google Scholar