State of the art of semi-analytic models

Semi-analytic models of galaxy formation and evolution are a powerful method to study how galaxies form and evolve within individual dark matter halos in a Λ-CDM cosmogony. We present the state of the art of current semi-analytic models, focusing on those properties of the galaxy population that are...

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Autor principal: Cora, Sofía Alejandra
Formato: Objeto de conferencia
Lenguaje:Español
Publicado: 2011
Materias:
Ciencias Astronómicas
Semi-analytic models
galaxy
properties
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/165341
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-165341
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spelling I19-R120-10915-1653412024-04-26T20:38:11Z http://sedici.unlp.edu.ar/handle/10915/165341 State of the art of semi-analytic models Cora, Sofía Alejandra 2011-11 2013 2024-04-26T12:41:18Z es Ciencias Astronómicas Semi-analytic models galaxy properties Semi-analytic models of galaxy formation and evolution are a powerful method to study how galaxies form and evolve within individual dark matter halos in a Λ-CDM cosmogony. We present the state of the art of current semi-analytic models, focusing on those properties of the galaxy population that are not properly reproduced by the model, which give hints of the astrophysical processes that still need better understanding. Facultad de Ciencias Astronómicas y Geofísicas Objeto de conferencia Objeto de conferencia http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 49-56
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Ciencias Astronómicas
Semi-analytic models
galaxy
properties
spellingShingle Ciencias Astronómicas
Semi-analytic models
galaxy
properties
Cora, Sofía Alejandra
State of the art of semi-analytic models
topic_facet Ciencias Astronómicas
Semi-analytic models
galaxy
properties
description Semi-analytic models of galaxy formation and evolution are a powerful method to study how galaxies form and evolve within individual dark matter halos in a Λ-CDM cosmogony. We present the state of the art of current semi-analytic models, focusing on those properties of the galaxy population that are not properly reproduced by the model, which give hints of the astrophysical processes that still need better understanding.
format Objeto de conferencia
Objeto de conferencia
author Cora, Sofía Alejandra
author_facet Cora, Sofía Alejandra
author_sort Cora, Sofía Alejandra
title State of the art of semi-analytic models
title_short State of the art of semi-analytic models
title_full State of the art of semi-analytic models
title_fullStr State of the art of semi-analytic models
title_full_unstemmed State of the art of semi-analytic models
title_sort state of the art of semi-analytic models
publishDate 2011
url http://sedici.unlp.edu.ar/handle/10915/165341
work_keys_str_mv AT corasofiaalejandra stateoftheartofsemianalyticmodels
_version_ 1807223042888171520

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