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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/30153
Ver los metadatos del registro completo
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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 Técnicas2025-09-29T10:26:07Zoai: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:34982025-09-29 10:26:08.259CONICET 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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13.070432 |