Hostname: page-component-848d4c4894-xfwgj Total loading time: 0 Render date: 2024-06-15T21:22:44.453Z Has data issue: false hasContentIssue false

Ratio of Early to Late Type Stars in SMC Clusters

Published online by Cambridge University Press:  19 July 2016

E. Kontizas
Affiliation:
Observatory of Athens.
M. Kontizas
Affiliation:
University of Athens.
A. Dapergolas
Affiliation:
Observatory of Athens.
D. Hatzidmitriou
Affiliation:
University of Edinburgh.

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.

Spectral classification of stars in SMC clusters provide useful information on the evolutionary history of this galaxy and permit us to test the theory of stellar evolution.

Type
Chapter VIII. Poster Papers on Cluster Systems in Nearby Galaxies
Copyright
Copyright © Kluwer 1988 

References

REFERENCES

Carney, B. W., Janes, K. A., Flower, P. J. 1985 Astron. J. 90, 7.Google Scholar
Dapergolas, A., Kontizas, E., Kontizas, M. 1986 Astron. Astrophys. Suppl., 65, 283.Google Scholar
Hodge, P. W. 1982 IAU Colloq. No. 68, p. 295.Google Scholar
Kontizas, E., Dapergolas, A., Kontizas, M. 1986 Astron. Astrophys. Suppl., 66, 51.Google Scholar
Kontizas, M. 1984 Astron. Astrophys. 131, 58.Google Scholar
Mould, J., Aaronson, M. 1982 Astrophys. J. 263, 629.CrossRefGoogle Scholar
Schlesinger, B. M. 1969 Astrophys. J. 157, 533.CrossRefGoogle Scholar
Schlesinger, B. M. 1971 Astrophys. J. 166, 447.Google Scholar