Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxies

Autores
Zandivarez, Arnaldo Ariel; Díaz Giménez, Eugenia; Taverna, Maria Antonela; Mamon, Gary
Año de publicación
2023
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Using over 3000 compact groups (CGs) of galaxies extracted from mock catalogues built from semi-analytical models (SAMs) of galaxy formation, we study whether the CG assembly channel affects the z = 0 properties of galaxies and their evolution. The evolution of CG galaxy properties with time is a clear function of their stellar masses. For instance, high-stellar-mass CG galaxies have lived their last 8 Gyr with little cold gas content while maintaining their reservoir of hot gas, while low-mass CG galaxies still preserve some of their cold gas content at the present but they have completely drained their hot gas reservoir. Beyond that, we find that the evolution of CG galaxies is also a function of the assembly history of the CGs: with more extreme losses of gas content, faster mass gain rates for black holes and more marked suppression of star formation as a function of cosmic time as we go from recent to early CG assembly. Thus, CGs constitute another laboratory for galaxy assembly bias, as the later assembling groups have later star formation. Our results show that classifying CGs according to their assembly channel is a way of distinguishing different paths by which galaxies transform their properties throughout their history.
Fil: Zandivarez, Arnaldo Ariel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Díaz Giménez, Eugenia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Taverna, Maria Antonela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Mamon, Gary. Institut d’Astrophysique de Paris; Francia
Materia
METHODS: DATA ANALYSIS
METHODS: NUMERICAL
METHODS: STATISTICAL
GALAXIES: GROUPS: GENERAL
GALAXIES: INTERACTIONS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/248421
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxiesZandivarez, Arnaldo ArielDíaz Giménez, EugeniaTaverna, Maria AntonelaMamon, GaryMETHODS: DATA ANALYSISMETHODS: NUMERICALMETHODS: STATISTICALGALAXIES: GROUPS: GENERALGALAXIES: INTERACTIONShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Using over 3000 compact groups (CGs) of galaxies extracted from mock catalogues built from semi-analytical models (SAMs) of galaxy formation, we study whether the CG assembly channel affects the z = 0 properties of galaxies and their evolution. The evolution of CG galaxy properties with time is a clear function of their stellar masses. For instance, high-stellar-mass CG galaxies have lived their last 8 Gyr with little cold gas content while maintaining their reservoir of hot gas, while low-mass CG galaxies still preserve some of their cold gas content at the present but they have completely drained their hot gas reservoir. Beyond that, we find that the evolution of CG galaxies is also a function of the assembly history of the CGs: with more extreme losses of gas content, faster mass gain rates for black holes and more marked suppression of star formation as a function of cosmic time as we go from recent to early CG assembly. Thus, CGs constitute another laboratory for galaxy assembly bias, as the later assembling groups have later star formation. Our results show that classifying CGs according to their assembly channel is a way of distinguishing different paths by which galaxies transform their properties throughout their history.Fil: Zandivarez, Arnaldo Ariel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Díaz Giménez, Eugenia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Taverna, Maria Antonela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Mamon, Gary. Institut d’Astrophysique de Paris; FranciaOxford University Press2023-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/248421Zandivarez, Arnaldo Ariel; Díaz Giménez, Eugenia; Taverna, Maria Antonela; Mamon, Gary; Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxies; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 526; 3; 12-2023; 3697-37150035-87111365-2966CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/526/3/3697/7287609info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad2986info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/2309.16764info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:05:58Zoai:ri.conicet.gov.ar:11336/248421instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:05:58.978CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxies
title Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxies
spellingShingle Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxies
Zandivarez, Arnaldo Ariel
METHODS: DATA ANALYSIS
METHODS: NUMERICAL
METHODS: STATISTICAL
GALAXIES: GROUPS: GENERAL
GALAXIES: INTERACTIONS
title_short Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxies
title_full Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxies
title_fullStr Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxies
title_full_unstemmed Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxies
title_sort Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxies
dc.creator.none.fl_str_mv Zandivarez, Arnaldo Ariel
Díaz Giménez, Eugenia
Taverna, Maria Antonela
Mamon, Gary
author Zandivarez, Arnaldo Ariel
author_facet Zandivarez, Arnaldo Ariel
Díaz Giménez, Eugenia
Taverna, Maria Antonela
Mamon, Gary
author_role author
author2 Díaz Giménez, Eugenia
Taverna, Maria Antonela
Mamon, Gary
author2_role author
author
author
dc.subject.none.fl_str_mv METHODS: DATA ANALYSIS
METHODS: NUMERICAL
METHODS: STATISTICAL
GALAXIES: GROUPS: GENERAL
GALAXIES: INTERACTIONS
topic METHODS: DATA ANALYSIS
METHODS: NUMERICAL
METHODS: STATISTICAL
GALAXIES: GROUPS: GENERAL
GALAXIES: INTERACTIONS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Using over 3000 compact groups (CGs) of galaxies extracted from mock catalogues built from semi-analytical models (SAMs) of galaxy formation, we study whether the CG assembly channel affects the z = 0 properties of galaxies and their evolution. The evolution of CG galaxy properties with time is a clear function of their stellar masses. For instance, high-stellar-mass CG galaxies have lived their last 8 Gyr with little cold gas content while maintaining their reservoir of hot gas, while low-mass CG galaxies still preserve some of their cold gas content at the present but they have completely drained their hot gas reservoir. Beyond that, we find that the evolution of CG galaxies is also a function of the assembly history of the CGs: with more extreme losses of gas content, faster mass gain rates for black holes and more marked suppression of star formation as a function of cosmic time as we go from recent to early CG assembly. Thus, CGs constitute another laboratory for galaxy assembly bias, as the later assembling groups have later star formation. Our results show that classifying CGs according to their assembly channel is a way of distinguishing different paths by which galaxies transform their properties throughout their history.
Fil: Zandivarez, Arnaldo Ariel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Díaz Giménez, Eugenia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Taverna, Maria Antonela. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Mamon, Gary. Institut d’Astrophysique de Paris; Francia
description Using over 3000 compact groups (CGs) of galaxies extracted from mock catalogues built from semi-analytical models (SAMs) of galaxy formation, we study whether the CG assembly channel affects the z = 0 properties of galaxies and their evolution. The evolution of CG galaxy properties with time is a clear function of their stellar masses. For instance, high-stellar-mass CG galaxies have lived their last 8 Gyr with little cold gas content while maintaining their reservoir of hot gas, while low-mass CG galaxies still preserve some of their cold gas content at the present but they have completely drained their hot gas reservoir. Beyond that, we find that the evolution of CG galaxies is also a function of the assembly history of the CGs: with more extreme losses of gas content, faster mass gain rates for black holes and more marked suppression of star formation as a function of cosmic time as we go from recent to early CG assembly. Thus, CGs constitute another laboratory for galaxy assembly bias, as the later assembling groups have later star formation. Our results show that classifying CGs according to their assembly channel is a way of distinguishing different paths by which galaxies transform their properties throughout their history.
publishDate 2023
dc.date.none.fl_str_mv 2023-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/248421
Zandivarez, Arnaldo Ariel; Díaz Giménez, Eugenia; Taverna, Maria Antonela; Mamon, Gary; Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxies; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 526; 3; 12-2023; 3697-3715
0035-8711
1365-2966
CONICET Digital
CONICET
url http://hdl.handle.net/11336/248421
identifier_str_mv Zandivarez, Arnaldo Ariel; Díaz Giménez, Eugenia; Taverna, Maria Antonela; Mamon, Gary; Compact groups from semi-analytical models of galaxy formation – IV: Effect of group assembly on the evolution of their galaxies; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 526; 3; 12-2023; 3697-3715
0035-8711
1365-2966
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/526/3/3697/7287609
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad2986
info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/2309.16764
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv Oxford University Press
publisher.none.fl_str_mv Oxford University Press
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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