Influence of the black hole rotation on accretion discs and jets in active galaxies: the case of NGC 1068

Detalhes bibliográficos
Autor(a) principal: Caproni,Anderson
Data de Publicação: 2005
Outros Autores: Abraham,Zulema, Cuesta,Herman J.Mosquera
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Brazilian Journal of Physics
Texto Completo: http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332005000700044
Resumo: Although we do not observe directly black holes in the Universe, their presence has been inferred in several astrophysical systems, from galactic to extragalactic scales. In this work, we will restrict our focus in the possible signatures of the presence of Kerr black holes in active galactic nuclei, one of the most powerful sources in the Universe. Particularly, we will discuss how jet/accretion disc precession and their directional stability can be used to trace the accretion disc properties as well as the black hole spin in the Seyfert galaxy NGC 1068.
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spelling Influence of the black hole rotation on accretion discs and jets in active galaxies: the case of NGC 1068Although we do not observe directly black holes in the Universe, their presence has been inferred in several astrophysical systems, from galactic to extragalactic scales. In this work, we will restrict our focus in the possible signatures of the presence of Kerr black holes in active galactic nuclei, one of the most powerful sources in the Universe. Particularly, we will discuss how jet/accretion disc precession and their directional stability can be used to trace the accretion disc properties as well as the black hole spin in the Seyfert galaxy NGC 1068.Sociedade Brasileira de Física2005-12-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersiontext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332005000700044Brazilian Journal of Physics v.35 n.4b 2005reponame:Brazilian Journal of Physicsinstname:Sociedade Brasileira de Física (SBF)instacron:SBF10.1590/S0103-97332005000700044info:eu-repo/semantics/openAccessCaproni,AndersonAbraham,ZulemaCuesta,Herman J.Mosqueraeng2006-01-18T00:00:00Zoai:scielo:S0103-97332005000700044Revistahttp://www.sbfisica.org.br/v1/home/index.php/pt/ONGhttps://old.scielo.br/oai/scielo-oai.phpsbfisica@sbfisica.org.br||sbfisica@sbfisica.org.br1678-44480103-9733opendoar:2006-01-18T00:00Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF)false
dc.title.none.fl_str_mv Influence of the black hole rotation on accretion discs and jets in active galaxies: the case of NGC 1068
title Influence of the black hole rotation on accretion discs and jets in active galaxies: the case of NGC 1068
spellingShingle Influence of the black hole rotation on accretion discs and jets in active galaxies: the case of NGC 1068
Caproni,Anderson
title_short Influence of the black hole rotation on accretion discs and jets in active galaxies: the case of NGC 1068
title_full Influence of the black hole rotation on accretion discs and jets in active galaxies: the case of NGC 1068
title_fullStr Influence of the black hole rotation on accretion discs and jets in active galaxies: the case of NGC 1068
title_full_unstemmed Influence of the black hole rotation on accretion discs and jets in active galaxies: the case of NGC 1068
title_sort Influence of the black hole rotation on accretion discs and jets in active galaxies: the case of NGC 1068
author Caproni,Anderson
author_facet Caproni,Anderson
Abraham,Zulema
Cuesta,Herman J.Mosquera
author_role author
author2 Abraham,Zulema
Cuesta,Herman J.Mosquera
author2_role author
author
dc.contributor.author.fl_str_mv Caproni,Anderson
Abraham,Zulema
Cuesta,Herman J.Mosquera
description Although we do not observe directly black holes in the Universe, their presence has been inferred in several astrophysical systems, from galactic to extragalactic scales. In this work, we will restrict our focus in the possible signatures of the presence of Kerr black holes in active galactic nuclei, one of the most powerful sources in the Universe. Particularly, we will discuss how jet/accretion disc precession and their directional stability can be used to trace the accretion disc properties as well as the black hole spin in the Seyfert galaxy NGC 1068.
publishDate 2005
dc.date.none.fl_str_mv 2005-12-01
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332005000700044
url http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332005000700044
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 10.1590/S0103-97332005000700044
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv text/html
dc.publisher.none.fl_str_mv Sociedade Brasileira de Física
publisher.none.fl_str_mv Sociedade Brasileira de Física
dc.source.none.fl_str_mv Brazilian Journal of Physics v.35 n.4b 2005
reponame:Brazilian Journal of Physics
instname:Sociedade Brasileira de Física (SBF)
instacron:SBF
instname_str Sociedade Brasileira de Física (SBF)
instacron_str SBF
institution SBF
reponame_str Brazilian Journal of Physics
collection Brazilian Journal of Physics
repository.name.fl_str_mv Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF)
repository.mail.fl_str_mv sbfisica@sbfisica.org.br||sbfisica@sbfisica.org.br
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