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Stellar populations of dwarf elliptical galaxies from high-resolution, optical spectroscopic data
Published online by Cambridge University Press: 01 December 2006
Abstract
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We present some preliminary results obtained within the MAGPOP-ITP collaboration for a subsample of four dwarf elliptical galaxies. On the basis of high-resolution, optical spectroscopic data obtained for these galaxies at the WHT, their ages, metallicities and single element abundance ratios have been derived from their line-strength indices and the improved, MILES-based, stellar population model predictions by Vazdekis et al. (in preparation).
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 430 - 431
- Copyright
- Copyright © International Astronomical Union 2007
References
Cenarro, A. J.; Peletier, R. F.; Sánchez-Blázquez, P.; Selam, S.; Toloba, E.; Cardiel, N.; Falcón-Barroso, J.; Gorgas, J.; Jiménez-Vicente, J.; & Vazdekis, A. 2007, MNRAS 374, 664CrossRefGoogle Scholar
Sánchez-Blázquez, P.; Peletier, R. F.; Jiménez-Vicente, J.; Cardiel, N.; Cenarro, A. J.; Falcón-Barroso, J.; Gorgas, J.; Selam, S.; & Vazdekis, A. 2006, MNRAS 371, 703CrossRefGoogle Scholar
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