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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

E. Toloba
Affiliation:
Dpto. de Física de la Tierra, Astronomía y Astrofísica II, Fac. de Ciencias Físicas, Universidad Complutense de Madrid, 28040 Madrid, Spain email: [email protected], [email protected]
J. Gorgas
Affiliation:
Dpto. de Física de la Tierra, Astronomía y Astrofísica II, Fac. de Ciencias Físicas, Universidad Complutense de Madrid, 28040 Madrid, Spain email: [email protected], [email protected]
A. J. Cenarro
Affiliation:
Instituto de Astrofísica de Canarias, Vía Láctea s/n, 38200 La Laguna, Tenerife, Spain email: [email protected]
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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
Copyright
Copyright © International Astronomical Union 2007

References

Cardiel, N. 1999, PhD Thesis, Universidad Complutense de Madrid, SpainGoogle Scholar
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
Vazdekis, A. et al. 2007, in preparationGoogle Scholar