Black Hole Ejected from the Nucleus of Galaxy NGC 5236

Autores
Dottori, H.; Diaz, Ruben Joaquin; Albacete Colombo, J. F.; Mast, D.
Año de publicación
2010
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The Fanaroff-Riley II-type radiosource J 133658.3-295105, which is also an X-ray source, appears to be projected onto the disc of the barred-spiral galaxy NGC 5236 (M 83) at about 1.2 kiloparsecs from the galaxy´s optical nucleus. J 133658.3-295105, its radio-lobes, and two other radiosources, neither of which are supernovae remnants or HII regions, are aligned with the optical nucleus of NGC 5236. Due to this peculiar on-the-sky projection, we studied J 133658.3-295105 using GEMINI+GMOS optical spectroscopy and also reanalyzed Chandra spectroscopy which was carried out in 2000. We marginally detected the Hα emission line receding at 130 km/sec with respect to the optical nucleus. We also demostrate that J 133658.3-295105 presents the Fe-Kα emission line at a redshift z = 0.018 ± 0.01. Both, Hα and Fe-Kα present redshifts that are compatible with the distance of NGC 5236. That findings reinforce the scenario of a local object for J 133658.3-295105, which could have been ejected from the nucleus of NGC 5236.
Fil: Dottori, H.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Diaz, Ruben Joaquin. Gemini Observatory; Estados Unidos. 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, J. F.. Universidad Nacional del Comahue; Argentina
Fil: Mast, D.. Centro Astronómico Hispano Alemán; España
Materia
Black Holes
Galactic Nucleus
Ngc 5236 Galaxy
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:11336/12971

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network_name_str CONICET Digital (CONICET)
spelling Black Hole Ejected from the Nucleus of Galaxy NGC 5236Dottori, H.Diaz, Ruben JoaquinAlbacete Colombo, J. F.Mast, D.Black HolesGalactic NucleusNgc 5236 Galaxyhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The Fanaroff-Riley II-type radiosource J 133658.3-295105, which is also an X-ray source, appears to be projected onto the disc of the barred-spiral galaxy NGC 5236 (M 83) at about 1.2 kiloparsecs from the galaxy´s optical nucleus. J 133658.3-295105, its radio-lobes, and two other radiosources, neither of which are supernovae remnants or HII regions, are aligned with the optical nucleus of NGC 5236. Due to this peculiar on-the-sky projection, we studied J 133658.3-295105 using GEMINI+GMOS optical spectroscopy and also reanalyzed Chandra spectroscopy which was carried out in 2000. We marginally detected the Hα emission line receding at 130 km/sec with respect to the optical nucleus. We also demostrate that J 133658.3-295105 presents the Fe-Kα emission line at a redshift z = 0.018 ± 0.01. Both, Hα and Fe-Kα present redshifts that are compatible with the distance of NGC 5236. That findings reinforce the scenario of a local object for J 133658.3-295105, which could have been ejected from the nucleus of NGC 5236.Fil: Dottori, H.. Universidade Federal do Rio Grande do Sul; BrasilFil: Diaz, Ruben Joaquin. Gemini Observatory; Estados Unidos. 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, J. F.. Universidad Nacional del Comahue; ArgentinaFil: Mast, D.. Centro Astronómico Hispano Alemán; EspañaWorld Scientific2010-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/12971Dottori, H.; Diaz, Ruben Joaquin; Albacete Colombo, J. F.; Mast, D.; Black Hole Ejected from the Nucleus of Galaxy NGC 5236; World Scientific; International Journal Of Modern Physics D; 19; 8; 12-2010; 1259-12640218-2718enginfo:eu-repo/semantics/altIdentifier/url/http://www.worldscientific.com/doi/abs/10.1142/S0218271810017494?journalCode=ijmpdinfo:eu-repo/semantics/altIdentifier/doi/10.1142/S0218271810017494info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:23:19Zoai:ri.conicet.gov.ar:11336/12971instacron: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:34982025-10-15 14:23:19.649CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Black Hole Ejected from the Nucleus of Galaxy NGC 5236
title Black Hole Ejected from the Nucleus of Galaxy NGC 5236
spellingShingle Black Hole Ejected from the Nucleus of Galaxy NGC 5236
Dottori, H.
Black Holes
Galactic Nucleus
Ngc 5236 Galaxy
title_short Black Hole Ejected from the Nucleus of Galaxy NGC 5236
title_full Black Hole Ejected from the Nucleus of Galaxy NGC 5236
title_fullStr Black Hole Ejected from the Nucleus of Galaxy NGC 5236
title_full_unstemmed Black Hole Ejected from the Nucleus of Galaxy NGC 5236
title_sort Black Hole Ejected from the Nucleus of Galaxy NGC 5236
dc.creator.none.fl_str_mv Dottori, H.
Diaz, Ruben Joaquin
Albacete Colombo, J. F.
Mast, D.
author Dottori, H.
author_facet Dottori, H.
Diaz, Ruben Joaquin
Albacete Colombo, J. F.
Mast, D.
author_role author
author2 Diaz, Ruben Joaquin
Albacete Colombo, J. F.
Mast, D.
author2_role author
author
author
dc.subject.none.fl_str_mv Black Holes
Galactic Nucleus
Ngc 5236 Galaxy
topic Black Holes
Galactic Nucleus
Ngc 5236 Galaxy
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-type radiosource J 133658.3-295105, which is also an X-ray source, appears to be projected onto the disc of the barred-spiral galaxy NGC 5236 (M 83) at about 1.2 kiloparsecs from the galaxy´s optical nucleus. J 133658.3-295105, its radio-lobes, and two other radiosources, neither of which are supernovae remnants or HII regions, are aligned with the optical nucleus of NGC 5236. Due to this peculiar on-the-sky projection, we studied J 133658.3-295105 using GEMINI+GMOS optical spectroscopy and also reanalyzed Chandra spectroscopy which was carried out in 2000. We marginally detected the Hα emission line receding at 130 km/sec with respect to the optical nucleus. We also demostrate that J 133658.3-295105 presents the Fe-Kα emission line at a redshift z = 0.018 ± 0.01. Both, Hα and Fe-Kα present redshifts that are compatible with the distance of NGC 5236. That findings reinforce the scenario of a local object for J 133658.3-295105, which could have been ejected from the nucleus of NGC 5236.
Fil: Dottori, H.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Diaz, Ruben Joaquin. Gemini Observatory; Estados Unidos. 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, J. F.. Universidad Nacional del Comahue; Argentina
Fil: Mast, D.. Centro Astronómico Hispano Alemán; España
description The Fanaroff-Riley II-type radiosource J 133658.3-295105, which is also an X-ray source, appears to be projected onto the disc of the barred-spiral galaxy NGC 5236 (M 83) at about 1.2 kiloparsecs from the galaxy´s optical nucleus. J 133658.3-295105, its radio-lobes, and two other radiosources, neither of which are supernovae remnants or HII regions, are aligned with the optical nucleus of NGC 5236. Due to this peculiar on-the-sky projection, we studied J 133658.3-295105 using GEMINI+GMOS optical spectroscopy and also reanalyzed Chandra spectroscopy which was carried out in 2000. We marginally detected the Hα emission line receding at 130 km/sec with respect to the optical nucleus. We also demostrate that J 133658.3-295105 presents the Fe-Kα emission line at a redshift z = 0.018 ± 0.01. Both, Hα and Fe-Kα present redshifts that are compatible with the distance of NGC 5236. That findings reinforce the scenario of a local object for J 133658.3-295105, which could have been ejected from the nucleus of NGC 5236.
publishDate 2010
dc.date.none.fl_str_mv 2010-12
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/11336/12971
Dottori, H.; Diaz, Ruben Joaquin; Albacete Colombo, J. F.; Mast, D.; Black Hole Ejected from the Nucleus of Galaxy NGC 5236; World Scientific; International Journal Of Modern Physics D; 19; 8; 12-2010; 1259-1264
0218-2718
url http://hdl.handle.net/11336/12971
identifier_str_mv Dottori, H.; Diaz, Ruben Joaquin; Albacete Colombo, J. F.; Mast, D.; Black Hole Ejected from the Nucleus of Galaxy NGC 5236; World Scientific; International Journal Of Modern Physics D; 19; 8; 12-2010; 1259-1264
0218-2718
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://www.worldscientific.com/doi/abs/10.1142/S0218271810017494?journalCode=ijmpd
info:eu-repo/semantics/altIdentifier/doi/10.1142/S0218271810017494
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 World Scientific
publisher.none.fl_str_mv World Scientific
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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