Effects of galaxy formation on dark matter haloes
We have studied six galaxy-sized haloes of the Aquarius Project, finding, in agreement with previous results, that baryon condensation leads to an increase of the dark matter concentration. We find that in all cases the velocity dispersion increases monotonically with radius. The shape and concentra...
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v40_n_p82_Pedrosa http://hdl.handle.net/20.500.12110/paper_14052059_v40_n_p82_Pedrosa |
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paper:paper_14052059_v40_n_p82_Pedrosa2023-06-08T16:13:24Z Effects of galaxy formation on dark matter haloes Cosmology: Theory Galaxies: Evolution Galaxies: Formation We have studied six galaxy-sized haloes of the Aquarius Project, finding, in agreement with previous results, that baryon condensation leads to an increase of the dark matter concentration. We find that in all cases the velocity dispersion increases monotonically with radius. The shape and concentration of the dark matter density profiles in ΔCDM universes are not well reproduced by adiabatic contraction models. © 2011: Instituto de Astronomía. 2011 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v40_n_p82_Pedrosa http://hdl.handle.net/20.500.12110/paper_14052059_v40_n_p82_Pedrosa |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Cosmology: Theory Galaxies: Evolution Galaxies: Formation |
spellingShingle |
Cosmology: Theory Galaxies: Evolution Galaxies: Formation Effects of galaxy formation on dark matter haloes |
topic_facet |
Cosmology: Theory Galaxies: Evolution Galaxies: Formation |
description |
We have studied six galaxy-sized haloes of the Aquarius Project, finding, in agreement with previous results, that baryon condensation leads to an increase of the dark matter concentration. We find that in all cases the velocity dispersion increases monotonically with radius. The shape and concentration of the dark matter density profiles in ΔCDM universes are not well reproduced by adiabatic contraction models. © 2011: Instituto de Astronomía. |
title |
Effects of galaxy formation on dark matter haloes |
title_short |
Effects of galaxy formation on dark matter haloes |
title_full |
Effects of galaxy formation on dark matter haloes |
title_fullStr |
Effects of galaxy formation on dark matter haloes |
title_full_unstemmed |
Effects of galaxy formation on dark matter haloes |
title_sort |
effects of galaxy formation on dark matter haloes |
publishDate |
2011 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_14052059_v40_n_p82_Pedrosa http://hdl.handle.net/20.500.12110/paper_14052059_v40_n_p82_Pedrosa |
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1768546641545003008 |