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: | http://hdl.handle.net/20.500.12110/paper_14052059_v40_n_p82_Pedrosa |
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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 |
_version_ |
1807322239643680768 |