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A near-infrared view of AGB stars in nearby dwarf galaxies
Published online by Cambridge University Press: 13 April 2010
Abstract
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As part of our near-infrared photometric survey of nearby dwarf galaxies, we present recent results for Leo I and Leo II dwarf spheroidal galaxies. We selected O- and C-rich AGB stellar populations using two-color diagrams and compared their luminosity functions and star counts with the predictions of the most recent AGB theoretical models.
- Type
- Poster Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 345 - 346
- Copyright
- Copyright © International Astronomical Union 2010
References
Girardi, L. & Marigo, 2007, in: Kerschbaum, F., Charbonnel, C., & Wing, R. F. (eds), Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes, ASP Conf. Series, Vol. 378, p 20Google Scholar
Gullieuszik, M., Held, E. V., Rizzi, L., Girardi, L., Marigo, P., & Momany, Y. 2008, MNRAS, 388, 1185CrossRefGoogle Scholar
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