State of the art of semi-analytic models

Autores
Cora, Sofía Alejandra
Año de publicación
2011
Idioma
español castellano
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
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
Materia
Ciencias Astronómicas
Semi-analytic models
galaxy
properties
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/165341
Acceder
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network_name_str SEDICI (UNLP)
spelling State of the art of semi-analytic modelsCora, Sofía AlejandraCiencias AstronómicasSemi-analytic modelsgalaxypropertiesSemi-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 Geofísicas2011-11info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf49-56http://sedici.unlp.edu.ar/handle/10915/165341spainfo:eu-repo/semantics/altIdentifier/isbn/978-987-24948-1-0info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:24:51Zoai:sedici.unlp.edu.ar:10915/165341Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:24:51.923SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv State of the art of semi-analytic models
title State of the art of semi-analytic models
spellingShingle State of the art of semi-analytic models
Cora, Sofía Alejandra
Ciencias Astronómicas
Semi-analytic models
galaxy
properties
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
dc.creator.none.fl_str_mv Cora, Sofía Alejandra
author Cora, Sofía Alejandra
author_facet Cora, Sofía Alejandra
author_role author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Semi-analytic models
galaxy
properties
topic Ciencias Astronómicas
Semi-analytic models
galaxy
properties
dc.description.none.fl_txt_mv 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
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.
publishDate 2011
dc.date.none.fl_str_mv 2011-11
dc.type.none.fl_str_mv info:eu-repo/semantics/conferenceObject
info:eu-repo/semantics/publishedVersion
Objeto de conferencia
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
format conferenceObject
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/165341
url http://sedici.unlp.edu.ar/handle/10915/165341
dc.language.none.fl_str_mv spa
language spa
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/isbn/978-987-24948-1-0
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
49-56
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repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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