The tully-fisher relation in numerical simulations of structure formation

The Tully-Fisher Relation (TFR) is of fundamental importance for galaxy formation as it provides information about the relation between the baryonic content of galaxies and the depth of their dark halos potential wells. In recent years, it has been possible to study this relation at different redshi...

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Guardado en:
Detalles Bibliográficos
Publicado: 2009
Materias:
Cosmology: dark matter
Galaxies: evolution
Galaxies: formation
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v5_nS262_p327_DeRossi
http://hdl.handle.net/20.500.12110/paper_17439213_v5_nS262_p327_DeRossi
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_17439213_v5_nS262_p327_DeRossi
record_format dspace
spelling paper:paper_17439213_v5_nS262_p327_DeRossi2023-06-08T16:28:00Z The tully-fisher relation in numerical simulations of structure formation Cosmology: dark matter Galaxies: evolution Galaxies: formation The Tully-Fisher Relation (TFR) is of fundamental importance for galaxy formation as it provides information about the relation between the baryonic content of galaxies and the depth of their dark halos potential wells. In recent years, it has been possible to study this relation at different redshifts. However, there are still controversies about its origin and evolution. In this work, we try to address the origin of the Tully-Fisher Relation by employing cosmological hydrodynamical simulations. © International Astronomical Union 2010. 2009 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v5_nS262_p327_DeRossi http://hdl.handle.net/20.500.12110/paper_17439213_v5_nS262_p327_DeRossi
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: dark matter
Galaxies: evolution
Galaxies: formation
spellingShingle Cosmology: dark matter
Galaxies: evolution
Galaxies: formation
The tully-fisher relation in numerical simulations of structure formation
topic_facet Cosmology: dark matter
Galaxies: evolution
Galaxies: formation
description The Tully-Fisher Relation (TFR) is of fundamental importance for galaxy formation as it provides information about the relation between the baryonic content of galaxies and the depth of their dark halos potential wells. In recent years, it has been possible to study this relation at different redshifts. However, there are still controversies about its origin and evolution. In this work, we try to address the origin of the Tully-Fisher Relation by employing cosmological hydrodynamical simulations. © International Astronomical Union 2010.
title The tully-fisher relation in numerical simulations of structure formation
title_short The tully-fisher relation in numerical simulations of structure formation
title_full The tully-fisher relation in numerical simulations of structure formation
title_fullStr The tully-fisher relation in numerical simulations of structure formation
title_full_unstemmed The tully-fisher relation in numerical simulations of structure formation
title_sort tully-fisher relation in numerical simulations of structure formation
publishDate 2009
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v5_nS262_p327_DeRossi
http://hdl.handle.net/20.500.12110/paper_17439213_v5_nS262_p327_DeRossi
_version_ 1768546041650479104

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