Kinetic AGN feedback effects on cluster cool cores simulated using SPH
- Autores
- Barai, Paramita; Murante, Giuseppe; Borgani, Stefano; Gaspari, Massimo; Granato, Gian Luigi; Monaco, Pierluigi; Ragone Figueroa, Cinthia Judith
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We implement novel numerical models of AGN feedback in the SPH code gadget-3, where the energy from a supermassive black hole (BH) is coupled to the surrounding gas in the kinetic form. Gas particles lying inside a bi-conical volume around the BH are imparted a one-time velocity (10 000 km s-1) increment. We perform hydrodynamical simulations of isolated cluster (total mass 1014 h-1 M⊙), which is initially evolved to form a dense cool core, having central T ≤ 106 K. A BH resides at the cluster centre, and ejects energy. The feedback-driven fast wind undergoes shock with the slower moving gas, which causes the imparted kinetic energy to be thermalized. Bipolar bubble-like outflows form propagating radially outward to a distance of a few 100 kpc. The radial profiles of median gas properties are influenced by BH feedback in the inner regions (r < 20-50 kpc). BH kinetic feedback, with a large value of the feedback efficiency, depletes the inner cool gas and reduces the hot gas content, such that the initial cool core of the cluster is heated up within a time 1.9 Gyr, whereby the core median temperature rises to above 107 K, and the central entropy flattens. Our implementation of BH thermal feedback (using the same efficiency as kinetic), within the star formation model, cannot do this heating, where the cool core remains. The inclusion of cold gas accretion in the simulations produces naturally a duty cycle of the AGN with a periodicity of 100 Myr.
Fil: Barai, Paramita. Istituto Nazionale di Astrofisica; Italia. Consiglio Nazionale delle Ricerche; Italia
Fil: Murante, Giuseppe. Istituto Nazionale di Astrofisica; Italia. Consiglio Nazionale delle Ricerche; Italia
Fil: Borgani, Stefano. Istituto Nazionale di Astrofisica; Italia. Università degli Studi di Trieste; Italia. Istituto Nazionale di Fisica Nucleare; Italia. Consiglio Nazionale delle Ricerche; Italia
Fil: Gaspari, Massimo. University of Princeton; Estados Unidos
Fil: Granato, Gian Luigi. Istituto Nazionale di Astrofisica; Italia. Consiglio Nazionale delle Ricerche; Italia
Fil: Monaco, Pierluigi. Istituto Nazionale di Astrofisica; Italia. Università degli Studi di Trieste; Italia. Consiglio Nazionale delle Ricerche; Italia
Fil: Ragone Figueroa, Cinthia Judith. Istituto Nazionale di Astrofisica; Italia. Consiglio Nazionale delle Ricerche; Italia. 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 - Materia
-
BLACK HOLE PHYSICS
COSMOLOGY: THEORY
GALAXIES: CLUSTERS: GENERAL
GALAXIES: JETS
HYDRODYNAMICS
QUASARS: SUPERMASSIVE BLACK HOLES - 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:11336/183147
Ver los metadatos del registro completo
id |
CONICETDig_8127ea630a2c42dae5697fd5d447fbbd |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/183147 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
network_name_str |
CONICET Digital (CONICET) |
spelling |
Kinetic AGN feedback effects on cluster cool cores simulated using SPHBarai, ParamitaMurante, GiuseppeBorgani, StefanoGaspari, MassimoGranato, Gian LuigiMonaco, PierluigiRagone Figueroa, Cinthia JudithBLACK HOLE PHYSICSCOSMOLOGY: THEORYGALAXIES: CLUSTERS: GENERALGALAXIES: JETSHYDRODYNAMICSQUASARS: SUPERMASSIVE BLACK HOLEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We implement novel numerical models of AGN feedback in the SPH code gadget-3, where the energy from a supermassive black hole (BH) is coupled to the surrounding gas in the kinetic form. Gas particles lying inside a bi-conical volume around the BH are imparted a one-time velocity (10 000 km s-1) increment. We perform hydrodynamical simulations of isolated cluster (total mass 1014 h-1 M⊙), which is initially evolved to form a dense cool core, having central T ≤ 106 K. A BH resides at the cluster centre, and ejects energy. The feedback-driven fast wind undergoes shock with the slower moving gas, which causes the imparted kinetic energy to be thermalized. Bipolar bubble-like outflows form propagating radially outward to a distance of a few 100 kpc. The radial profiles of median gas properties are influenced by BH feedback in the inner regions (r < 20-50 kpc). BH kinetic feedback, with a large value of the feedback efficiency, depletes the inner cool gas and reduces the hot gas content, such that the initial cool core of the cluster is heated up within a time 1.9 Gyr, whereby the core median temperature rises to above 107 K, and the central entropy flattens. Our implementation of BH thermal feedback (using the same efficiency as kinetic), within the star formation model, cannot do this heating, where the cool core remains. The inclusion of cold gas accretion in the simulations produces naturally a duty cycle of the AGN with a periodicity of 100 Myr.Fil: Barai, Paramita. Istituto Nazionale di Astrofisica; Italia. Consiglio Nazionale delle Ricerche; ItaliaFil: Murante, Giuseppe. Istituto Nazionale di Astrofisica; Italia. Consiglio Nazionale delle Ricerche; ItaliaFil: Borgani, Stefano. Istituto Nazionale di Astrofisica; Italia. Università degli Studi di Trieste; Italia. Istituto Nazionale di Fisica Nucleare; Italia. Consiglio Nazionale delle Ricerche; ItaliaFil: Gaspari, Massimo. University of Princeton; Estados UnidosFil: Granato, Gian Luigi. Istituto Nazionale di Astrofisica; Italia. Consiglio Nazionale delle Ricerche; ItaliaFil: Monaco, Pierluigi. Istituto Nazionale di Astrofisica; Italia. Università degli Studi di Trieste; Italia. Consiglio Nazionale delle Ricerche; ItaliaFil: Ragone Figueroa, Cinthia Judith. Istituto Nazionale di Astrofisica; Italia. Consiglio Nazionale delle Ricerche; Italia. 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; ArgentinaWiley Blackwell Publishing, Inc2016-09-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/183147Barai, Paramita; Murante, Giuseppe; Borgani, Stefano; Gaspari, Massimo; Granato, Gian Luigi; et al.; Kinetic AGN feedback effects on cluster cool cores simulated using SPH; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 461; 2; 11-9-2016; 1548-15670035-87111365-2966CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/461/2/1548/2608490info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw1389info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1605.08051info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:47:13Zoai:ri.conicet.gov.ar:11336/183147instacron: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 10:47:13.761CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Kinetic AGN feedback effects on cluster cool cores simulated using SPH |
title |
Kinetic AGN feedback effects on cluster cool cores simulated using SPH |
spellingShingle |
Kinetic AGN feedback effects on cluster cool cores simulated using SPH Barai, Paramita BLACK HOLE PHYSICS COSMOLOGY: THEORY GALAXIES: CLUSTERS: GENERAL GALAXIES: JETS HYDRODYNAMICS QUASARS: SUPERMASSIVE BLACK HOLES |
title_short |
Kinetic AGN feedback effects on cluster cool cores simulated using SPH |
title_full |
Kinetic AGN feedback effects on cluster cool cores simulated using SPH |
title_fullStr |
Kinetic AGN feedback effects on cluster cool cores simulated using SPH |
title_full_unstemmed |
Kinetic AGN feedback effects on cluster cool cores simulated using SPH |
title_sort |
Kinetic AGN feedback effects on cluster cool cores simulated using SPH |
dc.creator.none.fl_str_mv |
Barai, Paramita Murante, Giuseppe Borgani, Stefano Gaspari, Massimo Granato, Gian Luigi Monaco, Pierluigi Ragone Figueroa, Cinthia Judith |
author |
Barai, Paramita |
author_facet |
Barai, Paramita Murante, Giuseppe Borgani, Stefano Gaspari, Massimo Granato, Gian Luigi Monaco, Pierluigi Ragone Figueroa, Cinthia Judith |
author_role |
author |
author2 |
Murante, Giuseppe Borgani, Stefano Gaspari, Massimo Granato, Gian Luigi Monaco, Pierluigi Ragone Figueroa, Cinthia Judith |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
BLACK HOLE PHYSICS COSMOLOGY: THEORY GALAXIES: CLUSTERS: GENERAL GALAXIES: JETS HYDRODYNAMICS QUASARS: SUPERMASSIVE BLACK HOLES |
topic |
BLACK HOLE PHYSICS COSMOLOGY: THEORY GALAXIES: CLUSTERS: GENERAL GALAXIES: JETS HYDRODYNAMICS QUASARS: SUPERMASSIVE BLACK HOLES |
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 implement novel numerical models of AGN feedback in the SPH code gadget-3, where the energy from a supermassive black hole (BH) is coupled to the surrounding gas in the kinetic form. Gas particles lying inside a bi-conical volume around the BH are imparted a one-time velocity (10 000 km s-1) increment. We perform hydrodynamical simulations of isolated cluster (total mass 1014 h-1 M⊙), which is initially evolved to form a dense cool core, having central T ≤ 106 K. A BH resides at the cluster centre, and ejects energy. The feedback-driven fast wind undergoes shock with the slower moving gas, which causes the imparted kinetic energy to be thermalized. Bipolar bubble-like outflows form propagating radially outward to a distance of a few 100 kpc. The radial profiles of median gas properties are influenced by BH feedback in the inner regions (r < 20-50 kpc). BH kinetic feedback, with a large value of the feedback efficiency, depletes the inner cool gas and reduces the hot gas content, such that the initial cool core of the cluster is heated up within a time 1.9 Gyr, whereby the core median temperature rises to above 107 K, and the central entropy flattens. Our implementation of BH thermal feedback (using the same efficiency as kinetic), within the star formation model, cannot do this heating, where the cool core remains. The inclusion of cold gas accretion in the simulations produces naturally a duty cycle of the AGN with a periodicity of 100 Myr. Fil: Barai, Paramita. Istituto Nazionale di Astrofisica; Italia. Consiglio Nazionale delle Ricerche; Italia Fil: Murante, Giuseppe. Istituto Nazionale di Astrofisica; Italia. Consiglio Nazionale delle Ricerche; Italia Fil: Borgani, Stefano. Istituto Nazionale di Astrofisica; Italia. Università degli Studi di Trieste; Italia. Istituto Nazionale di Fisica Nucleare; Italia. Consiglio Nazionale delle Ricerche; Italia Fil: Gaspari, Massimo. University of Princeton; Estados Unidos Fil: Granato, Gian Luigi. Istituto Nazionale di Astrofisica; Italia. Consiglio Nazionale delle Ricerche; Italia Fil: Monaco, Pierluigi. Istituto Nazionale di Astrofisica; Italia. Università degli Studi di Trieste; Italia. Consiglio Nazionale delle Ricerche; Italia Fil: Ragone Figueroa, Cinthia Judith. Istituto Nazionale di Astrofisica; Italia. Consiglio Nazionale delle Ricerche; Italia. 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 |
description |
We implement novel numerical models of AGN feedback in the SPH code gadget-3, where the energy from a supermassive black hole (BH) is coupled to the surrounding gas in the kinetic form. Gas particles lying inside a bi-conical volume around the BH are imparted a one-time velocity (10 000 km s-1) increment. We perform hydrodynamical simulations of isolated cluster (total mass 1014 h-1 M⊙), which is initially evolved to form a dense cool core, having central T ≤ 106 K. A BH resides at the cluster centre, and ejects energy. The feedback-driven fast wind undergoes shock with the slower moving gas, which causes the imparted kinetic energy to be thermalized. Bipolar bubble-like outflows form propagating radially outward to a distance of a few 100 kpc. The radial profiles of median gas properties are influenced by BH feedback in the inner regions (r < 20-50 kpc). BH kinetic feedback, with a large value of the feedback efficiency, depletes the inner cool gas and reduces the hot gas content, such that the initial cool core of the cluster is heated up within a time 1.9 Gyr, whereby the core median temperature rises to above 107 K, and the central entropy flattens. Our implementation of BH thermal feedback (using the same efficiency as kinetic), within the star formation model, cannot do this heating, where the cool core remains. The inclusion of cold gas accretion in the simulations produces naturally a duty cycle of the AGN with a periodicity of 100 Myr. |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016-09-11 |
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/11336/183147 Barai, Paramita; Murante, Giuseppe; Borgani, Stefano; Gaspari, Massimo; Granato, Gian Luigi; et al.; Kinetic AGN feedback effects on cluster cool cores simulated using SPH; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 461; 2; 11-9-2016; 1548-1567 0035-8711 1365-2966 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/183147 |
identifier_str_mv |
Barai, Paramita; Murante, Giuseppe; Borgani, Stefano; Gaspari, Massimo; Granato, Gian Luigi; et al.; Kinetic AGN feedback effects on cluster cool cores simulated using SPH; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 461; 2; 11-9-2016; 1548-1567 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/461/2/1548/2608490 info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw1389 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1605.08051 |
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 |
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 |
_version_ |
1844614515629490176 |
score |
13.070432 |