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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/234296
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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 Técnicas2025-09-29T09:53:19Zoai: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:34982025-09-29 09:53:19.984CONICET 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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1844613629931945984 |
score |
13.070432 |