Hostname: page-component-77c89778f8-m42fx Total loading time: 0 Render date: 2024-07-20T07:32:15.627Z Has data issue: false hasContentIssue false
  • English
  • Français

Nonuniform Star Population of the LMC Cluster NGC 1978?

Published online by Cambridge University Press:  25 May 2016

V. Kravtsov
V. Kravtsov*
Affiliation:
Sternberg Astron. Inst., 13, University Ave., Moscow 119899, Russia

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.

The LMC cluster NGC 1978 shows different properties in the two parts divided by its minor axis. These two parts have different color distributions of the core He-burning (CHB) stars and giant branch (GB) positions on the CMDs at and below the level of the CHB stars. These differences may be caused by spread in metallicity.

Type
Part 6. Stellar Clusters
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 434 - 435
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Alcaino, G., Liller, W., Alvarado, F., et al. 1999, A&AS, 135, 103 Google Scholar
Bertelli, G., Bressan, A., Chiosi, C., et al. 1994, A&AS, 106, 275 Google Scholar
Bhatia, R. K., Read, M. A., Hatzidimitriou, D., et al. 1991, A&AS, 87, 335 Google Scholar
Bica, E., Claria, J. J., & Dottori, H. 1992, AJ, 103, 1859 Google Scholar
Fischer, P., Welch, D. L., & Mateo, M. 1992, AJ, 104, 1086 Google Scholar