Volume 388, Number 2, June III 2002
|Page(s)||396 - 406|
|Section||Cosmology (including clusters of galaxies)|
|Published online||31 May 2002|
Enhancement of α-elements in dynamical models of elliptical galaxies
Department of Astronomy, University of Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
2 Visiting Scientist, ESO, Karl-Schwarzschild-str. 2, 85748, Garching bei Muenchen, Germany e-mail: firstname.lastname@example.org; email@example.com
Corresponding author: R. Tantalo, firstname.lastname@example.org
Accepted: 19 March 2002
In this paper we present a quantitative analysis of the chemical abundances in “monolithic” N-body-Tree-SPH models of elliptical galaxies to determine whether the ratio increases with the galaxy mass as suggested by observational data.
Key words: galaxies: abundances / galaxies: elliptical and lenticular, cD / galaxies: evolution
© ESO, 2002
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