Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273

Autores
Torres, Diego F.; Romero, Gustavo Esteban; Barcons, Xavier; Lu, Youjun
Año de publicación
2003
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We propose the study of long-term variations in the Fe Ka line profile as a discriminator for binary black hole (BH) systems. The existence of a binary BH in the center of an active galaxy will produce a particular signature in the evolution of the line profile, as a result of disk precession. This signature is a periodic variation of the position of the blue edge of the profile, accompanied by periodic change of its intensity. We show that detection of the former is clearly within the observational capabilities of planned X-ray missions. Detecting a periodic variation of line profiles would provide the first direct evidence for precessing disks in active galactic nuclei, as opposed to the existing evidence supporting only the precession of jets. We apply these ideas to 3C 273.
Fil: Torres, Diego F.. Lawrence Livermore National Laboratory; Estados Unidos
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Barcons, Xavier. Instituto de física de cantabria; España
Fil: Lu, Youjun. University of Toronto; Canadá
Materia
Accretion disks
Black holes
Quasars
3C 273 (cuásar)
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/30153
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273Torres, Diego F.Romero, Gustavo EstebanBarcons, XavierLu, YoujunAccretion disksBlack holesQuasars3C 273 (cuásar)https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We propose the study of long-term variations in the Fe Ka line profile as a discriminator for binary black hole (BH) systems. The existence of a binary BH in the center of an active galaxy will produce a particular signature in the evolution of the line profile, as a result of disk precession. This signature is a periodic variation of the position of the blue edge of the profile, accompanied by periodic change of its intensity. We show that detection of the former is clearly within the observational capabilities of planned X-ray missions. Detecting a periodic variation of line profiles would provide the first direct evidence for precessing disks in active galactic nuclei, as opposed to the existing evidence supporting only the precession of jets. We apply these ideas to 3C 273.Fil: Torres, Diego F.. Lawrence Livermore National Laboratory; Estados UnidosFil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Barcons, Xavier. Instituto de física de cantabria; EspañaFil: Lu, Youjun. University of Toronto; CanadáIOP Publishing2003-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/30153Torres, Diego F.; Romero, Gustavo Esteban; Barcons, Xavier; Lu, Youjun; Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273; IOP Publishing; Astrophysical Journal; 596; 12-2003; 31-340004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1086/379108info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:58:50Zoai:ri.conicet.gov.ar:11336/30153instacron: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:34982025-10-22 11:58:50.55CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273
title Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273
spellingShingle Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273
Torres, Diego F.
Accretion disks
Black holes
Quasars
3C 273 (cuásar)
title_short Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273
title_full Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273
title_fullStr Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273
title_full_unstemmed Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273
title_sort Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273
dc.creator.none.fl_str_mv Torres, Diego F.
Romero, Gustavo Esteban
Barcons, Xavier
Lu, Youjun
author Torres, Diego F.
author_facet Torres, Diego F.
Romero, Gustavo Esteban
Barcons, Xavier
Lu, Youjun
author_role author
author2 Romero, Gustavo Esteban
Barcons, Xavier
Lu, Youjun
author2_role author
author
author
dc.subject.none.fl_str_mv Accretion disks
Black holes
Quasars
3C 273 (cuásar)
topic Accretion disks
Black holes
Quasars
3C 273 (cuásar)
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 propose the study of long-term variations in the Fe Ka line profile as a discriminator for binary black hole (BH) systems. The existence of a binary BH in the center of an active galaxy will produce a particular signature in the evolution of the line profile, as a result of disk precession. This signature is a periodic variation of the position of the blue edge of the profile, accompanied by periodic change of its intensity. We show that detection of the former is clearly within the observational capabilities of planned X-ray missions. Detecting a periodic variation of line profiles would provide the first direct evidence for precessing disks in active galactic nuclei, as opposed to the existing evidence supporting only the precession of jets. We apply these ideas to 3C 273.
Fil: Torres, Diego F.. Lawrence Livermore National Laboratory; Estados Unidos
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Barcons, Xavier. Instituto de física de cantabria; España
Fil: Lu, Youjun. University of Toronto; Canadá
description We propose the study of long-term variations in the Fe Ka line profile as a discriminator for binary black hole (BH) systems. The existence of a binary BH in the center of an active galaxy will produce a particular signature in the evolution of the line profile, as a result of disk precession. This signature is a periodic variation of the position of the blue edge of the profile, accompanied by periodic change of its intensity. We show that detection of the former is clearly within the observational capabilities of planned X-ray missions. Detecting a periodic variation of line profiles would provide the first direct evidence for precessing disks in active galactic nuclei, as opposed to the existing evidence supporting only the precession of jets. We apply these ideas to 3C 273.
publishDate 2003
dc.date.none.fl_str_mv 2003-12
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/11336/30153
Torres, Diego F.; Romero, Gustavo Esteban; Barcons, Xavier; Lu, Youjun; Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273; IOP Publishing; Astrophysical Journal; 596; 12-2003; 31-34
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/30153
identifier_str_mv Torres, Diego F.; Romero, Gustavo Esteban; Barcons, Xavier; Lu, Youjun; Testing the binary black hole paradigm through the Fe K alfha line profile : application to 3C 273; IOP Publishing; Astrophysical Journal; 596; 12-2003; 31-34
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1086/379108
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 IOP Publishing
publisher.none.fl_str_mv IOP Publishing
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
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score 12.982451

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