Hostname: page-component-8448b6f56d-gtxcr Total loading time: 0 Render date: 2024-04-25T05:42:17.232Z Has data issue: false hasContentIssue false
  • English
  • Français

Red Giant Stars in Magellanic Cloud Clusters: Constraining Population Synthesis Models

Published online by Cambridge University Press:  25 May 2016

Léo Girardi
Léo Girardi*
Affiliation:
Max-Planck-Institut für Astrophysik, Garching bei München, Germany

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.

We have developed a population synthesis code, aimed mainly at the interpretation of CMDs. Magellanic Cloud clusters have been largely used for the test/calibration of the underlying stellar tracks.

Type
Part 5. Stellar Populations and Surveys
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 374 - 376
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Bertelli, G., Bressan, A., Chiosi, C., et al. 1994, A&AS, 106, 275 Google Scholar
Corsi, C.E., Buonanno, R., Fusi Pecci, F., et al. 1994, MNRAS, 271, 385 Google Scholar
Girardi, L., Chiosi, C., Bertelli, G., & Bressan, A. 1995, A&A, 298, 87 Google Scholar
Girardi, L., & Bertelli, G. 1998, MNRAS, 300, 533 CrossRefGoogle Scholar
Girardi, L., Groenewegen, M.A.T., Weiss, A., et al. 1998, MNRAS, 301, 149 Google Scholar
Girardi, L., Bressan, A., Bertelli, G., & Chiosi, C. 1999, in preparation Google Scholar
Marigo, P., Girardi, L., & Chiosi, C. 1996, A&A, 316, L1 Google Scholar
Udalski, A. 1998, AcA, 48, 383 Google Scholar
Vassiliadis, E., & Wood, P.R. 1993, ApJ, 413, 641 CrossRefGoogle Scholar