The runaway black hole GRO J1655-40

Autores
Mirabel Miquele, Igor Felix; Mignani, R.; Rodrigues, I.; Combi, Jorge Ariel; Rodríguez, L. F.
Año de publicación
2002
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We have used the Hubble Space Telescope to measure the motion in the sky and compute the galactocentric orbit of the black hole X-ray binary GRO J1655-40. The system moves with a runaway space velocity of 112+/- 18 km s-1 in a highly eccentric (e = 0.34+/- 0.05) orbit. The black hole was formed in the disk at a distance greater than 3 kpc from the Galactic centre and must have been shot to such an eccentric orbit by the explosion of the progenitor star. The runaway linear momentum and kinetic energy of this black hole binary are comparable to those of solitary neutron stars and millisecond pulsars. GRO J1655-40 is the first black hole for which there is evidence for a runaway motion imparted by a natal kick in a supernova explosion. Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA, Inc. under contract No NAS 5-26555.
Fil: Mirabel Miquele, Igor Felix. Centre D; Francia
Fil: Mignani, R.. European Southern Observatory; Alemania
Fil: Rodrigues, I.. Centre D; Francia
Fil: Combi, Jorge Ariel. 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: Rodríguez, L. F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; México
Materia
GRO J1655-40 (estrella)
Black holes
X ray binaries
Astrometry
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:11336/30305
Acceder
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network_name_str CONICET Digital (CONICET)
spelling The runaway black hole GRO J1655-40Mirabel Miquele, Igor FelixMignani, R.Rodrigues, I.Combi, Jorge ArielRodríguez, L. F.GRO J1655-40 (estrella)Black holesX ray binariesAstrometryhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We have used the Hubble Space Telescope to measure the motion in the sky and compute the galactocentric orbit of the black hole X-ray binary GRO J1655-40. The system moves with a runaway space velocity of 112+/- 18 km s-1 in a highly eccentric (e = 0.34+/- 0.05) orbit. The black hole was formed in the disk at a distance greater than 3 kpc from the Galactic centre and must have been shot to such an eccentric orbit by the explosion of the progenitor star. The runaway linear momentum and kinetic energy of this black hole binary are comparable to those of solitary neutron stars and millisecond pulsars. GRO J1655-40 is the first black hole for which there is evidence for a runaway motion imparted by a natal kick in a supernova explosion. Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA, Inc. under contract No NAS 5-26555.Fil: Mirabel Miquele, Igor Felix. Centre D; FranciaFil: Mignani, R.. European Southern Observatory; AlemaniaFil: Rodrigues, I.. Centre D; FranciaFil: Combi, Jorge Ariel. 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: Rodríguez, L. F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; MéxicoEDP Sciences2002-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/30305Mirabel Miquele, Igor Felix; Mignani, R.; Rodrigues, I.; Combi, Jorge Ariel; Rodríguez, L. F.; The runaway black hole GRO J1655-40; EDP Sciences; Astronomy and Astrophysics; 395; 11-2002; 595-5990004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20021440info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2002/44/aa2903/aa2903.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T15:03:01Zoai:ri.conicet.gov.ar:11336/30305instacron: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 15:03:01.892CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The runaway black hole GRO J1655-40
title The runaway black hole GRO J1655-40
spellingShingle The runaway black hole GRO J1655-40
Mirabel Miquele, Igor Felix
GRO J1655-40 (estrella)
Black holes
X ray binaries
Astrometry
title_short The runaway black hole GRO J1655-40
title_full The runaway black hole GRO J1655-40
title_fullStr The runaway black hole GRO J1655-40
title_full_unstemmed The runaway black hole GRO J1655-40
title_sort The runaway black hole GRO J1655-40
dc.creator.none.fl_str_mv Mirabel Miquele, Igor Felix
Mignani, R.
Rodrigues, I.
Combi, Jorge Ariel
Rodríguez, L. F.
author Mirabel Miquele, Igor Felix
author_facet Mirabel Miquele, Igor Felix
Mignani, R.
Rodrigues, I.
Combi, Jorge Ariel
Rodríguez, L. F.
author_role author
author2 Mignani, R.
Rodrigues, I.
Combi, Jorge Ariel
Rodríguez, L. F.
author2_role author
author
author
author
dc.subject.none.fl_str_mv GRO J1655-40 (estrella)
Black holes
X ray binaries
Astrometry
topic GRO J1655-40 (estrella)
Black holes
X ray binaries
Astrometry
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 have used the Hubble Space Telescope to measure the motion in the sky and compute the galactocentric orbit of the black hole X-ray binary GRO J1655-40. The system moves with a runaway space velocity of 112+/- 18 km s-1 in a highly eccentric (e = 0.34+/- 0.05) orbit. The black hole was formed in the disk at a distance greater than 3 kpc from the Galactic centre and must have been shot to such an eccentric orbit by the explosion of the progenitor star. The runaway linear momentum and kinetic energy of this black hole binary are comparable to those of solitary neutron stars and millisecond pulsars. GRO J1655-40 is the first black hole for which there is evidence for a runaway motion imparted by a natal kick in a supernova explosion. Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA, Inc. under contract No NAS 5-26555.
Fil: Mirabel Miquele, Igor Felix. Centre D; Francia
Fil: Mignani, R.. European Southern Observatory; Alemania
Fil: Rodrigues, I.. Centre D; Francia
Fil: Combi, Jorge Ariel. 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: Rodríguez, L. F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; México
description We have used the Hubble Space Telescope to measure the motion in the sky and compute the galactocentric orbit of the black hole X-ray binary GRO J1655-40. The system moves with a runaway space velocity of 112+/- 18 km s-1 in a highly eccentric (e = 0.34+/- 0.05) orbit. The black hole was formed in the disk at a distance greater than 3 kpc from the Galactic centre and must have been shot to such an eccentric orbit by the explosion of the progenitor star. The runaway linear momentum and kinetic energy of this black hole binary are comparable to those of solitary neutron stars and millisecond pulsars. GRO J1655-40 is the first black hole for which there is evidence for a runaway motion imparted by a natal kick in a supernova explosion. Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA, Inc. under contract No NAS 5-26555.
publishDate 2002
dc.date.none.fl_str_mv 2002-11
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/11336/30305
Mirabel Miquele, Igor Felix; Mignani, R.; Rodrigues, I.; Combi, Jorge Ariel; Rodríguez, L. F.; The runaway black hole GRO J1655-40; EDP Sciences; Astronomy and Astrophysics; 395; 11-2002; 595-599
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/30305
identifier_str_mv Mirabel Miquele, Igor Felix; Mignani, R.; Rodrigues, I.; Combi, Jorge Ariel; Rodríguez, L. F.; The runaway black hole GRO J1655-40; EDP Sciences; Astronomy and Astrophysics; 395; 11-2002; 595-599
0004-6361
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20021440
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2002/44/aa2903/aa2903.html
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 EDP Sciences
publisher.none.fl_str_mv EDP Sciences
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 13.22299

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