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 CientiÂficas 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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/12971
Ver los metadatos del registro completo
id |
CONICETDig_8d459d9b65c662de57cc278528290616 |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/12971 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
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 CientiÂficas 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 CientiÂficas 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 |
_version_ |
1846082641425596416 |
score |
13.22299 |