Hostname: page-component-6bf8c574d5-2jptb Total loading time: 0 Render date: 2025-02-23T05:45:51.618Z Has data issue: false hasContentIssue false
  • English
  • Français

Monte Carlo simulations of globular cluster red giant branches

Published online by Cambridge University Press:  04 August 2017

Deborah A. Crocker  and
Robert T. Rood
Deborah A. Crocker
Affiliation:
Department of Astronomy, University of Virginia
Robert T. Rood
Affiliation:
Department of Astronomy, University of Virginia

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.

Simulations of globular cluster luminosity functions have shown that many of the features observed in actual clusters are probably statistical fluctuations. We suggest one new way of looking at the data which may ultimately lead to some information about the physical parameters of clusters.

Type
I. EVOLUTION OF LOW AND INTERMEDIATE MASS STARS OBSERVATIONS AND MODELS
Information
Symposium - International Astronomical Union , Volume 105: Observational Tests of the Stellar Evolution Theory , 1984 , pp. 159 - 161
Copyright
Copyright © Reidel 1984 

References

Buonanno, R., Buscema, C., Corsi, C. E. Iannicola, G., and Fusi-Pecci, F. 1983, Astr. Ap. Suppl., 51, 83.Google Scholar
Crocker, D. A., and Rood, R. T. (1984), in preparation.Google Scholar
Frogel, J. A., Persson, S. E., Cohen, J. G. 1981, in Astrophysical Processes in Red Giants, eds. Iben, I. and Renzini, A. (Dordrecht: Reidel), p. 55.Google Scholar
Rood, R. T. (1984), in preparation.Google Scholar