Hostname: page-component-848d4c4894-tn8tq Total loading time: 0 Render date: 2024-07-03T09:36:53.609Z Has data issue: false hasContentIssue false
  • English
  • Français

Photometric Models for Globular Clusters from Population Synthesis

Published online by Cambridge University Press:  19 July 2016

R. Capuzzo Dolcetta
R. Capuzzo Dolcetta*
Affiliation:
Astronomical Institute, Univ. of Rome

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.

Integral fluxes (Bolometric and U, B, V) are computed in a completely theoretical frame in order to investigate the structural properties and stellar content of coeval stellar systems of various ages and metal abundance. Some results concerning the problem of the color gap in the distribution of the sample of Magellanic Cloud clusters are discussed.

Type
Chapter VIII. Poster Papers on Cluster Systems in Nearby Galaxies
Information
Symposium - International Astronomical Union , Volume 126: The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies , 1988 , pp. 559 - 560
Copyright
Copyright © Kluwer 1988 

References

REFERENCES

Battinelli, P. and Capuzzo Dolcetta, R. 1986, in preparation.Google Scholar
Capuzzo Dolcetta, R. 1986 in Proc. of the Rome Astrophys. Coll., The Age of the Stellar Systems, in press.Google Scholar
Gascoigne, S. B. C. 1980 in IAU Symposium No. 85. Star Clusters, Hesser, J. E., ed., Reidel, Dordrecht, p. 305.Google Scholar
van den Bergh, S. 1981 Astron. Astrophys. Suppl. 46, 79.Google Scholar