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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Autores principales: Pedrosa, S.E., Tissera, P.B., Scannapieco, C.
Formato: CONF
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_14052059_v40_n_p82_Pedrosa
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spelling todo:paper_14052059_v40_n_p82_Pedrosa2023-10-03T16:13:02Z Effects of galaxy formation on dark matter haloes Pedrosa, S.E. Tissera, P.B. Scannapieco, C. 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. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar 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
Pedrosa, S.E.
Tissera, P.B.
Scannapieco, C.
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.
format CONF
author Pedrosa, S.E.
Tissera, P.B.
Scannapieco, C.
author_facet Pedrosa, S.E.
Tissera, P.B.
Scannapieco, C.
author_sort Pedrosa, S.E.
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
url http://hdl.handle.net/20.500.12110/paper_14052059_v40_n_p82_Pedrosa
work_keys_str_mv AT pedrosase effectsofgalaxyformationondarkmatterhaloes
AT tisserapb effectsofgalaxyformationondarkmatterhaloes
AT scannapiecoc effectsofgalaxyformationondarkmatterhaloes
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