The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters

Autores
Hough, Tomas; Cora, Sofia Alejandra; Haggar, Roan; Vega Martínez, Cristian Antonio; Kuchner, Ulrike; Pearce, Frazer; Gray, Meghan; Knebe, Alexander; Yepes, Gustavo
Año de publicación
2023
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In this work, we combine the semi-analytic model of galaxy formation and evolution SAG with the 102 relaxed simulated galaxy clusters from THE THREE HUNDRED project, and we study the link between the quenching of star formation (SF) and the physical processes that galaxies experience through their dynamical history in and around clusters. We classify galaxies in four populations based on their orbital history: recent and ancient infallers, and backsplash and neighbouring galaxies. We find that ∼85 per cent of the current population of quenched galaxies located inside the clusters are ancient infallers with low or null content of hot and cold gas. The fraction of quenched ancient infallers increases strongly between the first and second pericentric passage, due to the removal of hot gas by the action of ram-pressure stripping (RPS). The majority of them quenches after the first pericentric passage, but a non-negligible fraction needs a second passage, specially galaxies with M   ≤10^10.5 Msun . Recent infallers represent ∼15 per cent of the quenched galaxies located inside the cluster and, on av erage, the y contain a high proportion of hot and cold gas; moreover, pre-processing effects are responsible for quenching the recent inf allers prior to inf all onto the main cluster progenitor. The ∼65 per cent of quenched galaxies located around clusters are backsplash galaxies, for which the combination of RPS acting during a pre-processing stage and inside the cluster is necessary for the suppression of SF in this population.
Fil: Hough, Tomas. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Cora, Sofia Alejandra. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Haggar, Roan. The University Of Nottingham. School Of Physics & Astronomy; Reino Unido
Fil: Vega Martínez, Cristian Antonio. Universidad de La Serena; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Kuchner, Ulrike. The University Of Nottingham. School Of Physics & Astronomy; Reino Unido
Fil: Pearce, Frazer. The University Of Nottingham. School Of Physics & Astronomy; Reino Unido
Fil: Gray, Meghan. The University Of Nottingham. School Of Physics & Astronomy; Reino Unido
Fil: Knebe, Alexander. Universidad Autónoma de Madrid; España
Fil: Yepes, Gustavo. Universidad Autónoma de Madrid; España
Materia
methods: numerical
galaxies: clusters: general
galaxies: evolution
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:11336/234296
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clustersHough, TomasCora, Sofia AlejandraHaggar, RoanVega Martínez, Cristian AntonioKuchner, UlrikePearce, FrazerGray, MeghanKnebe, AlexanderYepes, Gustavomethods: numericalgalaxies: clusters: generalgalaxies: evolutionhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In this work, we combine the semi-analytic model of galaxy formation and evolution SAG with the 102 relaxed simulated galaxy clusters from THE THREE HUNDRED project, and we study the link between the quenching of star formation (SF) and the physical processes that galaxies experience through their dynamical history in and around clusters. We classify galaxies in four populations based on their orbital history: recent and ancient infallers, and backsplash and neighbouring galaxies. We find that ∼85 per cent of the current population of quenched galaxies located inside the clusters are ancient infallers with low or null content of hot and cold gas. The fraction of quenched ancient infallers increases strongly between the first and second pericentric passage, due to the removal of hot gas by the action of ram-pressure stripping (RPS). The majority of them quenches after the first pericentric passage, but a non-negligible fraction needs a second passage, specially galaxies with M   ≤10^10.5 Msun . Recent infallers represent ∼15 per cent of the quenched galaxies located inside the cluster and, on av erage, the y contain a high proportion of hot and cold gas; moreover, pre-processing effects are responsible for quenching the recent inf allers prior to inf all onto the main cluster progenitor. The ∼65 per cent of quenched galaxies located around clusters are backsplash galaxies, for which the combination of RPS acting during a pre-processing stage and inside the cluster is necessary for the suppression of SF in this population.Fil: Hough, Tomas. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Cora, Sofia Alejandra. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Haggar, Roan. The University Of Nottingham. School Of Physics & Astronomy; Reino UnidoFil: Vega Martínez, Cristian Antonio. Universidad de La Serena; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Kuchner, Ulrike. The University Of Nottingham. School Of Physics & Astronomy; Reino UnidoFil: Pearce, Frazer. The University Of Nottingham. School Of Physics & Astronomy; Reino UnidoFil: Gray, Meghan. The University Of Nottingham. School Of Physics & Astronomy; Reino UnidoFil: Knebe, Alexander. Universidad Autónoma de Madrid; EspañaFil: Yepes, Gustavo. Universidad Autónoma de Madrid; EspañaWiley Blackwell Publishing, Inc2023-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/234296Hough, Tomas; Cora, Sofia Alejandra; Haggar, Roan; Vega Martínez, Cristian Antonio; Kuchner, Ulrike; et al.; The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 518; 2; 1-2023; 2398-24170035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/518/2/2398/6815734info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stac3209info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:22:42Zoai:ri.conicet.gov.ar:11336/234296instacron: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:34982025-10-22 11:22:43.213CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
title The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
spellingShingle The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
Hough, Tomas
methods: numerical
galaxies: clusters: general
galaxies: evolution
title_short The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
title_full The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
title_fullStr The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
title_full_unstemmed The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
title_sort The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
dc.creator.none.fl_str_mv Hough, Tomas
Cora, Sofia Alejandra
Haggar, Roan
Vega Martínez, Cristian Antonio
Kuchner, Ulrike
Pearce, Frazer
Gray, Meghan
Knebe, Alexander
Yepes, Gustavo
author Hough, Tomas
author_facet Hough, Tomas
Cora, Sofia Alejandra
Haggar, Roan
Vega Martínez, Cristian Antonio
Kuchner, Ulrike
Pearce, Frazer
Gray, Meghan
Knebe, Alexander
Yepes, Gustavo
author_role author
author2 Cora, Sofia Alejandra
Haggar, Roan
Vega Martínez, Cristian Antonio
Kuchner, Ulrike
Pearce, Frazer
Gray, Meghan
Knebe, Alexander
Yepes, Gustavo
author2_role author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv methods: numerical
galaxies: clusters: general
galaxies: evolution
topic methods: numerical
galaxies: clusters: general
galaxies: evolution
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv In this work, we combine the semi-analytic model of galaxy formation and evolution SAG with the 102 relaxed simulated galaxy clusters from THE THREE HUNDRED project, and we study the link between the quenching of star formation (SF) and the physical processes that galaxies experience through their dynamical history in and around clusters. We classify galaxies in four populations based on their orbital history: recent and ancient infallers, and backsplash and neighbouring galaxies. We find that ∼85 per cent of the current population of quenched galaxies located inside the clusters are ancient infallers with low or null content of hot and cold gas. The fraction of quenched ancient infallers increases strongly between the first and second pericentric passage, due to the removal of hot gas by the action of ram-pressure stripping (RPS). The majority of them quenches after the first pericentric passage, but a non-negligible fraction needs a second passage, specially galaxies with M   ≤10^10.5 Msun . Recent infallers represent ∼15 per cent of the quenched galaxies located inside the cluster and, on av erage, the y contain a high proportion of hot and cold gas; moreover, pre-processing effects are responsible for quenching the recent inf allers prior to inf all onto the main cluster progenitor. The ∼65 per cent of quenched galaxies located around clusters are backsplash galaxies, for which the combination of RPS acting during a pre-processing stage and inside the cluster is necessary for the suppression of SF in this population.
Fil: Hough, Tomas. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Cora, Sofia Alejandra. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Haggar, Roan. The University Of Nottingham. School Of Physics & Astronomy; Reino Unido
Fil: Vega Martínez, Cristian Antonio. Universidad de La Serena; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Kuchner, Ulrike. The University Of Nottingham. School Of Physics & Astronomy; Reino Unido
Fil: Pearce, Frazer. The University Of Nottingham. School Of Physics & Astronomy; Reino Unido
Fil: Gray, Meghan. The University Of Nottingham. School Of Physics & Astronomy; Reino Unido
Fil: Knebe, Alexander. Universidad Autónoma de Madrid; España
Fil: Yepes, Gustavo. Universidad Autónoma de Madrid; España
description In this work, we combine the semi-analytic model of galaxy formation and evolution SAG with the 102 relaxed simulated galaxy clusters from THE THREE HUNDRED project, and we study the link between the quenching of star formation (SF) and the physical processes that galaxies experience through their dynamical history in and around clusters. We classify galaxies in four populations based on their orbital history: recent and ancient infallers, and backsplash and neighbouring galaxies. We find that ∼85 per cent of the current population of quenched galaxies located inside the clusters are ancient infallers with low or null content of hot and cold gas. The fraction of quenched ancient infallers increases strongly between the first and second pericentric passage, due to the removal of hot gas by the action of ram-pressure stripping (RPS). The majority of them quenches after the first pericentric passage, but a non-negligible fraction needs a second passage, specially galaxies with M   ≤10^10.5 Msun . Recent infallers represent ∼15 per cent of the quenched galaxies located inside the cluster and, on av erage, the y contain a high proportion of hot and cold gas; moreover, pre-processing effects are responsible for quenching the recent inf allers prior to inf all onto the main cluster progenitor. The ∼65 per cent of quenched galaxies located around clusters are backsplash galaxies, for which the combination of RPS acting during a pre-processing stage and inside the cluster is necessary for the suppression of SF in this population.
publishDate 2023
dc.date.none.fl_str_mv 2023-01
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/11336/234296
Hough, Tomas; Cora, Sofia Alejandra; Haggar, Roan; Vega Martínez, Cristian Antonio; Kuchner, Ulrike; et al.; The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 518; 2; 1-2023; 2398-2417
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/234296
identifier_str_mv Hough, Tomas; Cora, Sofia Alejandra; Haggar, Roan; Vega Martínez, Cristian Antonio; Kuchner, Ulrike; et al.; The Three Hundred Project: Connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 518; 2; 1-2023; 2398-2417
0035-8711
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/518/2/2398/6815734
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stac3209
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
dc.publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
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 12.982451

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