The three hundred project: The gas disruption of infalling objects in cluster environments
- Autores
- Mostoghiu, Robert; Arthur, Jake; Pearce, Frazer R.; Gray, Meghan; Knebe, Alexander; Cui, Weiguang; Welker, Charlotte; Cora, Sofia Alejandra; Murante, Giuseppe; Dolag, Klaus; Yepes, Gustavo
- Año de publicación
- 2021
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We analyse the gas content evolution of infalling haloes in cluster environments from THE THREE HUNDRED project, a collection of 324 numerically modelled galaxy clusters. The haloes in our sample were selected within 5R200 of the main cluster halo at z = 0 and have total halo mass M200 ≥ 1011h−1M⊙. We track their main progenitors and study their gas evolution since their crossing into the infall region, which we define as 1–4R200. Studying the radial trends of our populations using both the full phase-space information and a line-of-sight projection, we confirm the Arthur et al. (2019) result and identify a characteristic radius around 1.7R200 in 3D and at R200 in projection at which infalling haloes lose nearly all of the gas prior their infall. Splitting the trends by subhalo status,we show that subhaloes residing in group-mass and low-mass host haloes in the infall region follow similar radial gas-loss trends as their hosts, whereas subhaloes of cluster-mass host haloes are stripped of their gas much further out. Our results show that infalling objects suffer significant gaseous disruption that correlates with time-since-infall, cluster-centric distance, and host mass, and that the gaseous disruption they experience is a combination of subhalo pre-processing and object gas depletion at a radius that behaves like an accretion shock.
Fil: Mostoghiu, Robert. Universidad Autónoma de Madrid; España. University of Western Australia; Australia. University of Nottingham; Estados Unidos
Fil: Arthur, Jake. University of Nottingham; Estados Unidos
Fil: Pearce, Frazer R.. University of Nottingham; Estados Unidos
Fil: Gray, Meghan. University of Nottingham; Estados Unidos
Fil: Knebe, Alexander. Universidad Autónoma de Madrid; España. University of Western Australia; Australia
Fil: Cui, Weiguang. University of Edinburgh; Reino Unido
Fil: Welker, Charlotte. University Johns Hopkins; Estados Unidos. Mcmaster University; Canadá
Fil: Cora, Sofia Alejandra. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Observatorio Astronómico de La Plata - Sede Central; Argentina. 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: Murante, Giuseppe. Istituto Nazionale di Astrofisica; Italia
Fil: Dolag, Klaus. University Observatory Munich; Alemania. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania
Fil: Yepes, Gustavo. Universidad Autónoma de Madrid; España - Materia
-
GALAXIES: EVOLUTION
GALAXIES: INTERACTIONS
METHODS: NUMERICAL - 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:11336/145384
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The three hundred project: The gas disruption of infalling objects in cluster environmentsMostoghiu, RobertArthur, JakePearce, Frazer R.Gray, MeghanKnebe, AlexanderCui, WeiguangWelker, CharlotteCora, Sofia AlejandraMurante, GiuseppeDolag, KlausYepes, GustavoGALAXIES: EVOLUTIONGALAXIES: INTERACTIONSMETHODS: NUMERICALhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We analyse the gas content evolution of infalling haloes in cluster environments from THE THREE HUNDRED project, a collection of 324 numerically modelled galaxy clusters. The haloes in our sample were selected within 5R200 of the main cluster halo at z = 0 and have total halo mass M200 ≥ 1011h−1M⊙. We track their main progenitors and study their gas evolution since their crossing into the infall region, which we define as 1–4R200. Studying the radial trends of our populations using both the full phase-space information and a line-of-sight projection, we confirm the Arthur et al. (2019) result and identify a characteristic radius around 1.7R200 in 3D and at R200 in projection at which infalling haloes lose nearly all of the gas prior their infall. Splitting the trends by subhalo status,we show that subhaloes residing in group-mass and low-mass host haloes in the infall region follow similar radial gas-loss trends as their hosts, whereas subhaloes of cluster-mass host haloes are stripped of their gas much further out. Our results show that infalling objects suffer significant gaseous disruption that correlates with time-since-infall, cluster-centric distance, and host mass, and that the gaseous disruption they experience is a combination of subhalo pre-processing and object gas depletion at a radius that behaves like an accretion shock.Fil: Mostoghiu, Robert. Universidad Autónoma de Madrid; España. University of Western Australia; Australia. University of Nottingham; Estados UnidosFil: Arthur, Jake. University of Nottingham; Estados UnidosFil: Pearce, Frazer R.. University of Nottingham; Estados UnidosFil: Gray, Meghan. University of Nottingham; Estados UnidosFil: Knebe, Alexander. Universidad Autónoma de Madrid; España. University of Western Australia; AustraliaFil: Cui, Weiguang. University of Edinburgh; Reino UnidoFil: Welker, Charlotte. University Johns Hopkins; Estados Unidos. Mcmaster University; CanadáFil: Cora, Sofia Alejandra. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Observatorio Astronómico de La Plata - Sede Central; Argentina. 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: Murante, Giuseppe. Istituto Nazionale di Astrofisica; ItaliaFil: Dolag, Klaus. University Observatory Munich; Alemania. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; AlemaniaFil: Yepes, Gustavo. Universidad Autónoma de Madrid; EspañaOxford University Press2021-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/145384Mostoghiu, Robert; Arthur, Jake; Pearce, Frazer R.; Gray, Meghan; Knebe, Alexander; et al.; The three hundred project: The gas disruption of infalling objects in cluster environments; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 501; 4; 3-2021; 5029-50410035-87111365-2966CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stab014info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/501/4/5029/6067373info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:32:50Zoai:ri.conicet.gov.ar:11336/145384instacron: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 10:32:50.366CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The three hundred project: The gas disruption of infalling objects in cluster environments |
title |
The three hundred project: The gas disruption of infalling objects in cluster environments |
spellingShingle |
The three hundred project: The gas disruption of infalling objects in cluster environments Mostoghiu, Robert GALAXIES: EVOLUTION GALAXIES: INTERACTIONS METHODS: NUMERICAL |
title_short |
The three hundred project: The gas disruption of infalling objects in cluster environments |
title_full |
The three hundred project: The gas disruption of infalling objects in cluster environments |
title_fullStr |
The three hundred project: The gas disruption of infalling objects in cluster environments |
title_full_unstemmed |
The three hundred project: The gas disruption of infalling objects in cluster environments |
title_sort |
The three hundred project: The gas disruption of infalling objects in cluster environments |
dc.creator.none.fl_str_mv |
Mostoghiu, Robert Arthur, Jake Pearce, Frazer R. Gray, Meghan Knebe, Alexander Cui, Weiguang Welker, Charlotte Cora, Sofia Alejandra Murante, Giuseppe Dolag, Klaus Yepes, Gustavo |
author |
Mostoghiu, Robert |
author_facet |
Mostoghiu, Robert Arthur, Jake Pearce, Frazer R. Gray, Meghan Knebe, Alexander Cui, Weiguang Welker, Charlotte Cora, Sofia Alejandra Murante, Giuseppe Dolag, Klaus Yepes, Gustavo |
author_role |
author |
author2 |
Arthur, Jake Pearce, Frazer R. Gray, Meghan Knebe, Alexander Cui, Weiguang Welker, Charlotte Cora, Sofia Alejandra Murante, Giuseppe Dolag, Klaus Yepes, Gustavo |
author2_role |
author author author author author author author author author author |
dc.subject.none.fl_str_mv |
GALAXIES: EVOLUTION GALAXIES: INTERACTIONS METHODS: NUMERICAL |
topic |
GALAXIES: EVOLUTION GALAXIES: INTERACTIONS METHODS: NUMERICAL |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We analyse the gas content evolution of infalling haloes in cluster environments from THE THREE HUNDRED project, a collection of 324 numerically modelled galaxy clusters. The haloes in our sample were selected within 5R200 of the main cluster halo at z = 0 and have total halo mass M200 ≥ 1011h−1M⊙. We track their main progenitors and study their gas evolution since their crossing into the infall region, which we define as 1–4R200. Studying the radial trends of our populations using both the full phase-space information and a line-of-sight projection, we confirm the Arthur et al. (2019) result and identify a characteristic radius around 1.7R200 in 3D and at R200 in projection at which infalling haloes lose nearly all of the gas prior their infall. Splitting the trends by subhalo status,we show that subhaloes residing in group-mass and low-mass host haloes in the infall region follow similar radial gas-loss trends as their hosts, whereas subhaloes of cluster-mass host haloes are stripped of their gas much further out. Our results show that infalling objects suffer significant gaseous disruption that correlates with time-since-infall, cluster-centric distance, and host mass, and that the gaseous disruption they experience is a combination of subhalo pre-processing and object gas depletion at a radius that behaves like an accretion shock. Fil: Mostoghiu, Robert. Universidad Autónoma de Madrid; España. University of Western Australia; Australia. University of Nottingham; Estados Unidos Fil: Arthur, Jake. University of Nottingham; Estados Unidos Fil: Pearce, Frazer R.. University of Nottingham; Estados Unidos Fil: Gray, Meghan. University of Nottingham; Estados Unidos Fil: Knebe, Alexander. Universidad Autónoma de Madrid; España. University of Western Australia; Australia Fil: Cui, Weiguang. University of Edinburgh; Reino Unido Fil: Welker, Charlotte. University Johns Hopkins; Estados Unidos. Mcmaster University; Canadá Fil: Cora, Sofia Alejandra. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Observatorio Astronómico de La Plata - Sede Central; Argentina. 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: Murante, Giuseppe. Istituto Nazionale di Astrofisica; Italia Fil: Dolag, Klaus. University Observatory Munich; Alemania. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania Fil: Yepes, Gustavo. Universidad Autónoma de Madrid; España |
description |
We analyse the gas content evolution of infalling haloes in cluster environments from THE THREE HUNDRED project, a collection of 324 numerically modelled galaxy clusters. The haloes in our sample were selected within 5R200 of the main cluster halo at z = 0 and have total halo mass M200 ≥ 1011h−1M⊙. We track their main progenitors and study their gas evolution since their crossing into the infall region, which we define as 1–4R200. Studying the radial trends of our populations using both the full phase-space information and a line-of-sight projection, we confirm the Arthur et al. (2019) result and identify a characteristic radius around 1.7R200 in 3D and at R200 in projection at which infalling haloes lose nearly all of the gas prior their infall. Splitting the trends by subhalo status,we show that subhaloes residing in group-mass and low-mass host haloes in the infall region follow similar radial gas-loss trends as their hosts, whereas subhaloes of cluster-mass host haloes are stripped of their gas much further out. Our results show that infalling objects suffer significant gaseous disruption that correlates with time-since-infall, cluster-centric distance, and host mass, and that the gaseous disruption they experience is a combination of subhalo pre-processing and object gas depletion at a radius that behaves like an accretion shock. |
publishDate |
2021 |
dc.date.none.fl_str_mv |
2021-03 |
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/11336/145384 Mostoghiu, Robert; Arthur, Jake; Pearce, Frazer R.; Gray, Meghan; Knebe, Alexander; et al.; The three hundred project: The gas disruption of infalling objects in cluster environments; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 501; 4; 3-2021; 5029-5041 0035-8711 1365-2966 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/145384 |
identifier_str_mv |
Mostoghiu, Robert; Arthur, Jake; Pearce, Frazer R.; Gray, Meghan; Knebe, Alexander; et al.; The three hundred project: The gas disruption of infalling objects in cluster environments; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 501; 4; 3-2021; 5029-5041 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/doi/10.1093/mnras/stab014 info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/501/4/5029/6067373 |
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 |
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) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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1844614342680510464 |
score |
13.070432 |