No CrossRef data available.
Article contents
Observations of clusters with ages from 0.01 to 1.0 Gyr in the Large Magellanic Cloud
Published online by Cambridge University Press: 01 April 2008
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 stellar initial mass function (IMF) is a very important question in modern astrophysics. Globular clusters (GCs) are good samples for studying the IMF, but the Galactic GCs can provide only one time-scale evolutionary stage. The Large Magellanic Cloud (LMC) is an ideal environment for studying the IMF because it contains compact clusters at different evolutionary stages. By studying the IMF at different evolutionary stages, we can see how the mass function evolves with time.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Symposium S252: The Art of Modeling Stars in the 21st Century , April 2008 , pp. 121 - 122
- Copyright
- Copyright © International Astronomical Union 2008
References
de Grijs, R., Gilmore, G. F., Johnson, R. A., & Mackey, A. D 2002, MNRAS 331, 245CrossRefGoogle Scholar
Holtzman, J. A., Burrows, C. J., Casertano, S., Hester, J. J., Trauger, J. T., Watson, A. M., & Worthey, G. 1995, PASP 107, 1065CrossRefGoogle Scholar
You have
Access