IMBHs in globular clusters: Accretion rate correlations with cluster parameters

The existence of intermediate-mass black holes 102-103M☉ is still a matter of debate. However, since their presence in globular clusters could impact on our knowledge of these systems, IMBHs deserve a detailed study of their detection mechanisms. One of these mechanisms is the detection of the emiss...

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Publicado: 2013
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Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_1824016X_v84_n1_p133_Pepe
http://hdl.handle.net/20.500.12110/paper_1824016X_v84_n1_p133_Pepe
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spelling paper:paper_1824016X_v84_n1_p133_Pepe2023-06-08T16:29:15Z IMBHs in globular clusters: Accretion rate correlations with cluster parameters Accretion Black hole physics Globular clusters: general Giant stars Accretion Black Hole physics Cluster parameters Detection mechanism Globular clusters Globular clusters: general Gravitational potential Intermediate mass black holes Gravitation The existence of intermediate-mass black holes 102-103M☉ is still a matter of debate. However, since their presence in globular clusters could impact on our knowledge of these systems, IMBHs deserve a detailed study of their detection mechanisms. One of these mechanisms is the detection of the emission due to the accretion of the surrounding media. In this work we present a simple numerical model to estimate the accretion rate onto IMBHs at the centre of GCs in order to find correlations between this and the cluster parameters. Our model includes the gravitational potential of the cluster and the constant injection of gas by the red giants in the cluster. We find that, if IMBHs are actually present at the centres of GCs they would be more easily detectable in more massive clusters with large values of the stellar velocity dispersion. © SAIt 2013 2013 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_1824016X_v84_n1_p133_Pepe http://hdl.handle.net/20.500.12110/paper_1824016X_v84_n1_p133_Pepe
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Accretion
Black hole physics
Globular clusters: general
Giant stars
Accretion
Black Hole physics
Cluster parameters
Detection mechanism
Globular clusters
Globular clusters: general
Gravitational potential
Intermediate mass black holes
Gravitation
spellingShingle Accretion
Black hole physics
Globular clusters: general
Giant stars
Accretion
Black Hole physics
Cluster parameters
Detection mechanism
Globular clusters
Globular clusters: general
Gravitational potential
Intermediate mass black holes
Gravitation
IMBHs in globular clusters: Accretion rate correlations with cluster parameters
topic_facet Accretion
Black hole physics
Globular clusters: general
Giant stars
Accretion
Black Hole physics
Cluster parameters
Detection mechanism
Globular clusters
Globular clusters: general
Gravitational potential
Intermediate mass black holes
Gravitation
description The existence of intermediate-mass black holes 102-103M☉ is still a matter of debate. However, since their presence in globular clusters could impact on our knowledge of these systems, IMBHs deserve a detailed study of their detection mechanisms. One of these mechanisms is the detection of the emission due to the accretion of the surrounding media. In this work we present a simple numerical model to estimate the accretion rate onto IMBHs at the centre of GCs in order to find correlations between this and the cluster parameters. Our model includes the gravitational potential of the cluster and the constant injection of gas by the red giants in the cluster. We find that, if IMBHs are actually present at the centres of GCs they would be more easily detectable in more massive clusters with large values of the stellar velocity dispersion. © SAIt 2013
title IMBHs in globular clusters: Accretion rate correlations with cluster parameters
title_short IMBHs in globular clusters: Accretion rate correlations with cluster parameters
title_full IMBHs in globular clusters: Accretion rate correlations with cluster parameters
title_fullStr IMBHs in globular clusters: Accretion rate correlations with cluster parameters
title_full_unstemmed IMBHs in globular clusters: Accretion rate correlations with cluster parameters
title_sort imbhs in globular clusters: accretion rate correlations with cluster parameters
publishDate 2013
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_1824016X_v84_n1_p133_Pepe
http://hdl.handle.net/20.500.12110/paper_1824016X_v84_n1_p133_Pepe
_version_ 1768541676723240960