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Stellar populations of dwarf elliptical galaxies from high-resolution, optical spectroscopic data

  • E. Toloba (a1), J. Gorgas (a1), A. J. Cenarro (a2) and the MAGPOP-ITP team

Abstract

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).

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References

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Cardiel, N. 1999, PhD Thesis, Universidad Complutense de Madrid, Spain
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, 664
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, 703
Vazdekis, A. et al. 2007, in preparation
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Keywords

Stellar populations of dwarf elliptical galaxies from high-resolution, optical spectroscopic data

  • E. Toloba (a1), J. Gorgas (a1), A. J. Cenarro (a2) and the MAGPOP-ITP team

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