The Three Hundred project: the gas disruption of infalling objects in cluster environments
- Autores
- Mostoghiu, Robert; Arthur, Jake; Pearce, Frazer R.; Gray, Meghan E.; Knebe, Alexander; Cui, Weiguang; Welker, Charlotte; Cora, Sofía 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 which behaves like an accretion shock.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata - Materia
-
Astronomía
methods: numerical
galaxies: evolution
galaxies: interactions - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/125503
Ver los metadatos del registro completo
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The Three Hundred project: the gas disruption of infalling objects in cluster environmentsMostoghiu, RobertArthur, JakePearce, Frazer R.Gray, Meghan E.Knebe, AlexanderCui, WeiguangWelker, CharlotteCora, Sofía AlejandraMurante, GiuseppeDolag, KlausYepes, GustavoAstronomíamethods: numericalgalaxies: evolutiongalaxies: interactionsWe 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 which behaves like an accretion shock.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plata2021-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf5029-5041http://sedici.unlp.edu.ar/handle/10915/125503enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/issn/1365-2966info:eu-repo/semantics/altIdentifier/arxiv/2101.01734info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stab014info: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:UNLP2025-09-29T11:29:48Zoai:sedici.unlp.edu.ar:10915/125503Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:29:48.636SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| 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 Astronomía methods: numerical galaxies: evolution galaxies: interactions |
| 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 E. Knebe, Alexander Cui, Weiguang Welker, Charlotte Cora, Sofía Alejandra Murante, Giuseppe Dolag, Klaus Yepes, Gustavo |
| author |
Mostoghiu, Robert |
| author_facet |
Mostoghiu, Robert Arthur, Jake Pearce, Frazer R. Gray, Meghan E. Knebe, Alexander Cui, Weiguang Welker, Charlotte Cora, Sofía Alejandra Murante, Giuseppe Dolag, Klaus Yepes, Gustavo |
| author_role |
author |
| author2 |
Arthur, Jake Pearce, Frazer R. Gray, Meghan E. Knebe, Alexander Cui, Weiguang Welker, Charlotte Cora, Sofía 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 |
Astronomía methods: numerical galaxies: evolution galaxies: interactions |
| topic |
Astronomía methods: numerical galaxies: evolution galaxies: interactions |
| 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 which behaves like an accretion shock. Facultad de Ciencias Astronómicas y Geofísicas Instituto de Astrofísica de La Plata |
| 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 which behaves like an accretion shock. |
| publishDate |
2021 |
| dc.date.none.fl_str_mv |
2021-03 |
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http://sedici.unlp.edu.ar/handle/10915/125503 |
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eng |
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eng |
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