The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83

Autores
Dottori, Horacio; Diaz, Ruben Joaquin; Albacete Colombo, Juan Facundo; Mast, Damian
Año de publicación
2010
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The Fanaroff-Riley II radio source J133658.3-295105, which is also an X-ray source, appears to be projected onto the disk of the barred-spiral galaxy M83 at about 60´´ from the galaxy´s optical nucleus. J133658.3-295105 and its radio lobes are aligned with the optical nucleus of M 83 and two other radio sources, neither of which are supernova remnants or H II regions. Due to this peculiar on-the-sky projection, J133658.3-295105 was previously studied by Gemini+GMOS optical spectroscopy, which marginally revealed the presence of Hα in emission receding at 130 km s-1 with respect to the optical nucleus. In this Letter, we reanalyze the Chandra spectroscopy carried out in 2000. We show that J133658.3-295105 presents an Fe Kα emission line at a redshift of z = 0.018. This redshift is compatible with a black hole at the distance of M 83. We discuss similarities to the recently reported micro-quasar in NGC 5408. This finding reinforces the kicked-off black hole scenario for J133658.3-295105.
Fil: Dottori, Horacio. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Diaz, Ruben Joaquin. Gemini Observatory; Chile. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; Argentina
Fil: Albacete Colombo, Juan Facundo. Universidad Nacional del Comahue; Argentina
Fil: Mast, Damian. Centro Astronomico Hispano Alemán; España. Consejo Superior de Investigaciones Cientificas. Instituto de Astrofísica de Andalucía; España
Materia
Galaxies: Evolution
Galaxies: Kinematics And Dynamics
Galaxies: Nuclei
X-Rays: Individual: J 133658.3295105
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:11336/12997
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/12997
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83Dottori, HoracioDiaz, Ruben JoaquinAlbacete Colombo, Juan FacundoMast, DamianGalaxies: EvolutionGalaxies: Kinematics And DynamicsGalaxies: NucleiX-Rays: Individual: J 133658.3295105https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The Fanaroff-Riley II radio source J133658.3-295105, which is also an X-ray source, appears to be projected onto the disk of the barred-spiral galaxy M83 at about 60´´ from the galaxy´s optical nucleus. J133658.3-295105 and its radio lobes are aligned with the optical nucleus of M 83 and two other radio sources, neither of which are supernova remnants or H II regions. Due to this peculiar on-the-sky projection, J133658.3-295105 was previously studied by Gemini+GMOS optical spectroscopy, which marginally revealed the presence of Hα in emission receding at 130 km s-1 with respect to the optical nucleus. In this Letter, we reanalyze the Chandra spectroscopy carried out in 2000. We show that J133658.3-295105 presents an Fe Kα emission line at a redshift of z = 0.018. This redshift is compatible with a black hole at the distance of M 83. We discuss similarities to the recently reported micro-quasar in NGC 5408. This finding reinforces the kicked-off black hole scenario for J133658.3-295105.Fil: Dottori, Horacio. Universidade Federal do Rio Grande do Sul; BrasilFil: Diaz, Ruben Joaquin. Gemini Observatory; Chile. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; ArgentinaFil: Albacete Colombo, Juan Facundo. Universidad Nacional del Comahue; ArgentinaFil: Mast, Damian. Centro Astronomico Hispano Alemán; España. Consejo Superior de Investigaciones Cientificas. Instituto de Astrofísica de Andalucía; EspañaIop Publishing2010-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/12997Dottori, Horacio; Diaz, Ruben Joaquin; Albacete Colombo, Juan Facundo; Mast, Damian; The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83; Iop Publishing; Astrophysical Journal; 717; 1; 7-2010; 42-460004-637Xenginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/2041-8205/717/1/L42info:eu-repo/semantics/altIdentifier/url/https://doi.org/10.1088/2041-8205/717/1/L42info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:54:52Zoai:ri.conicet.gov.ar:11336/12997instacron: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 11:54:53.045CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83
title The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83
spellingShingle The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83
Dottori, Horacio
Galaxies: Evolution
Galaxies: Kinematics And Dynamics
Galaxies: Nuclei
X-Rays: Individual: J 133658.3295105
title_short The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83
title_full The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83
title_fullStr The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83
title_full_unstemmed The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83
title_sort The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83
dc.creator.none.fl_str_mv Dottori, Horacio
Diaz, Ruben Joaquin
Albacete Colombo, Juan Facundo
Mast, Damian
author Dottori, Horacio
author_facet Dottori, Horacio
Diaz, Ruben Joaquin
Albacete Colombo, Juan Facundo
Mast, Damian
author_role author
author2 Diaz, Ruben Joaquin
Albacete Colombo, Juan Facundo
Mast, Damian
author2_role author
author
author
dc.subject.none.fl_str_mv Galaxies: Evolution
Galaxies: Kinematics And Dynamics
Galaxies: Nuclei
X-Rays: Individual: J 133658.3295105
topic Galaxies: Evolution
Galaxies: Kinematics And Dynamics
Galaxies: Nuclei
X-Rays: Individual: J 133658.3295105
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The Fanaroff-Riley II radio source J133658.3-295105, which is also an X-ray source, appears to be projected onto the disk of the barred-spiral galaxy M83 at about 60´´ from the galaxy´s optical nucleus. J133658.3-295105 and its radio lobes are aligned with the optical nucleus of M 83 and two other radio sources, neither of which are supernova remnants or H II regions. Due to this peculiar on-the-sky projection, J133658.3-295105 was previously studied by Gemini+GMOS optical spectroscopy, which marginally revealed the presence of Hα in emission receding at 130 km s-1 with respect to the optical nucleus. In this Letter, we reanalyze the Chandra spectroscopy carried out in 2000. We show that J133658.3-295105 presents an Fe Kα emission line at a redshift of z = 0.018. This redshift is compatible with a black hole at the distance of M 83. We discuss similarities to the recently reported micro-quasar in NGC 5408. This finding reinforces the kicked-off black hole scenario for J133658.3-295105.
Fil: Dottori, Horacio. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Diaz, Ruben Joaquin. Gemini Observatory; Chile. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; Argentina
Fil: Albacete Colombo, Juan Facundo. Universidad Nacional del Comahue; Argentina
Fil: Mast, Damian. Centro Astronomico Hispano Alemán; España. Consejo Superior de Investigaciones Cientificas. Instituto de Astrofísica de Andalucía; España
description The Fanaroff-Riley II radio source J133658.3-295105, which is also an X-ray source, appears to be projected onto the disk of the barred-spiral galaxy M83 at about 60´´ from the galaxy´s optical nucleus. J133658.3-295105 and its radio lobes are aligned with the optical nucleus of M 83 and two other radio sources, neither of which are supernova remnants or H II regions. Due to this peculiar on-the-sky projection, J133658.3-295105 was previously studied by Gemini+GMOS optical spectroscopy, which marginally revealed the presence of Hα in emission receding at 130 km s-1 with respect to the optical nucleus. In this Letter, we reanalyze the Chandra spectroscopy carried out in 2000. We show that J133658.3-295105 presents an Fe Kα emission line at a redshift of z = 0.018. This redshift is compatible with a black hole at the distance of M 83. We discuss similarities to the recently reported micro-quasar in NGC 5408. This finding reinforces the kicked-off black hole scenario for J133658.3-295105.
publishDate 2010
dc.date.none.fl_str_mv 2010-07
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/11336/12997
Dottori, Horacio; Diaz, Ruben Joaquin; Albacete Colombo, Juan Facundo; Mast, Damian; The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83; Iop Publishing; Astrophysical Journal; 717; 1; 7-2010; 42-46
0004-637X
url http://hdl.handle.net/11336/12997
identifier_str_mv Dottori, Horacio; Diaz, Ruben Joaquin; Albacete Colombo, Juan Facundo; Mast, Damian; The Missing Goliath's Slingshot: Massive Black Hole Recoil at M83; Iop Publishing; Astrophysical Journal; 717; 1; 7-2010; 42-46
0004-637X
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/2041-8205/717/1/L42
info:eu-repo/semantics/altIdentifier/url/https://doi.org/10.1088/2041-8205/717/1/L42
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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