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Formation and evolution of dwarf elliptical galaxies: Structural and kinematical properties

Published online by Cambridge University Press:  08 November 2005

S. De Rijcke
Affiliation:
Sterrenkundig Observatorium, Ghent University, Krijgslaan 281, S9, B-9000 Gent, Belgium email: sven.derijcke@UGent.be
D. Michielsen
Affiliation:
Sterrenkundig Observatorium, Ghent University, Krijgslaan 281, S9, B-9000 Gent, Belgium email: sven.derijcke@UGent.be
H. Dejonghe
Affiliation:
Sterrenkundig Observatorium, Ghent University, Krijgslaan 281, S9, B-9000 Gent, Belgium email: sven.derijcke@UGent.be
W.W. Zeilinger
Affiliation:
Institut für Astronomie, Universität Wien, Türkenschanzstraße 17, A-1180 Wien, Austria
G.K.T. Hau
Affiliation:
Department of Physics, South Road, Durham, DH1 3LE, UK
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Abstract

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We confront predictions of the currently popular theories for dE formation and evolution with the observed position of dEs in $\log L_B$ vs. $\log \sigma$, $\log L_B$ vs. $\log R_{\rm e}$, $\log L_B$ vs. $\log I_{\rm e}$, and $\log R_{\rm e}$ vs. $\log I_{\rm e}$ diagrams and in the ($\log \sigma,\log R_{\rm e},\log I_{\rm e}$) parameter space in which bright and intermediate-luminosity elliptical galaxies and bulges of spirals define a Fundamental Plane (FP). We show that the dE sequences in the various univariate diagrams are disjunct from those traced by bright and intermediate-luminosity elliptical galaxies and bulges of spirals. It appears that semi-analytical models (SAMs) that incorporate quiescent star formation with an essentially $z$-independent star-formation efficiency, combined with post-merger starbursts and the dynamical response after supernova-driven gas-loss, are able to reproduce the position of the dEs in the various univariate and bivariate diagrams.

Type
Contributed Papers
Copyright
© 2005 International Astronomical Union