Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/19027
Title: Isolated dwarf galaxies: from cuspy to flat dark matter density profiles and metalicity gradients
Authors: Pasetto, S.
Grebel, E. K.
Berczik, P.
Spurzem, R.
Dehnen, W.
First Published: 1-May-2010
Publisher: EDP Sciences for European Southern Observatory (ESO)
Citation: Astronomy & Astrophysics, 2010, 514
Abstract: The chemodynamical evolution of spherical multi-component self-gravitating models for isolated dwarf galaxies is studied. We compared their evolution with and without feedback effects from star formation processes. We found that initially cuspy dark matter profiles flatten with time without any special tuning conditions as a result of star formation. Thus the seemingly flattened profiles found in many dwarfs do not contradict the cuspy profiles predicted by cosmological models. We also calculated the chemical evolution of stars and gas, to permit comparisons with observational data.
DOI Link: 10.1051/0004-6361/200913240
ISSN: 0004-6361
Links: http://hdl.handle.net/2381/19027
http://www.aanda.org/articles/aa/abs/2010/06/aa13240-09/aa13240-09.html
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2010 ESO. Reproduced with permission from Astronomy & Astrophysics, © ESO.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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