IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations

Autores
Pellizza González, Leonardo Javier; Chaty, S.; Negueruela, I.
Año de publicación
2006
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
One of the most recent discoveries of the INTEGRAL observatory is the existence of a previously unknown population of X-ray sources in the inner arms of the Galaxy. IGR J17544-2619, IGR J16465-4507 and XTE J1739-302 are among these sources. Although the nature of these systems is still unexplained, the investigations of the optical/NIR counterparts of the two last sources, combined with high energy data, have provided evidence of them being highly absorbed high mass X-ray binaries with blue supergiant secondaries and displaying fast X-ray transient behaviour. In this work we present our optical/NIR observations of IGR J17544-2619, aimed at identifying and characterizing its counterpart. We show that the source is a high mass X-ray binary at a distance of 2-4 kpc with a strongly absorbed O9Ib secondary, and discuss the nature of the system.
Fil: Pellizza González, Leonardo Javier. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universite Paris Diderot - Paris 7; Francia
Fil: Chaty, S.. Universite Paris Diderot - Paris 7; Francia
Fil: Negueruela, I.. Universidad de Alicante; España
Materia
X-RAYS: BINARIES
X-RAYS: INDIVIDUAL: IGR J17544-2619
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:11336/16672
Acceder
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network_name_str CONICET Digital (CONICET)
spelling IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observationsPellizza González, Leonardo JavierChaty, S.Negueruela, I.X-RAYS: BINARIESX-RAYS: INDIVIDUAL: IGR J17544-2619https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1One of the most recent discoveries of the INTEGRAL observatory is the existence of a previously unknown population of X-ray sources in the inner arms of the Galaxy. IGR J17544-2619, IGR J16465-4507 and XTE J1739-302 are among these sources. Although the nature of these systems is still unexplained, the investigations of the optical/NIR counterparts of the two last sources, combined with high energy data, have provided evidence of them being highly absorbed high mass X-ray binaries with blue supergiant secondaries and displaying fast X-ray transient behaviour. In this work we present our optical/NIR observations of IGR J17544-2619, aimed at identifying and characterizing its counterpart. We show that the source is a high mass X-ray binary at a distance of 2-4 kpc with a strongly absorbed O9Ib secondary, and discuss the nature of the system.Fil: Pellizza González, Leonardo Javier. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universite Paris Diderot - Paris 7; FranciaFil: Chaty, S.. Universite Paris Diderot - Paris 7; FranciaFil: Negueruela, I.. Universidad de Alicante; EspañaEdp Sciences2006-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/16672Pellizza González, Leonardo Javier; Chaty, S.; Negueruela, I.; IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations; Edp Sciences; Astronomy And Astrophysics; 455; 2; 8-2006; 653-6580004-6361enginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20054436info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2006/32/aa4436-05/aa4436-05.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 Técnicas2025-10-15T14:54:31Zoai:ri.conicet.gov.ar:11336/16672instacron: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 14:54:31.697CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations
title IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations
spellingShingle IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations
Pellizza González, Leonardo Javier
X-RAYS: BINARIES
X-RAYS: INDIVIDUAL: IGR J17544-2619
title_short IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations
title_full IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations
title_fullStr IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations
title_full_unstemmed IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations
title_sort IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations
dc.creator.none.fl_str_mv Pellizza González, Leonardo Javier
Chaty, S.
Negueruela, I.
author Pellizza González, Leonardo Javier
author_facet Pellizza González, Leonardo Javier
Chaty, S.
Negueruela, I.
author_role author
author2 Chaty, S.
Negueruela, I.
author2_role author
author
dc.subject.none.fl_str_mv X-RAYS: BINARIES
X-RAYS: INDIVIDUAL: IGR J17544-2619
topic X-RAYS: BINARIES
X-RAYS: INDIVIDUAL: IGR J17544-2619
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv One of the most recent discoveries of the INTEGRAL observatory is the existence of a previously unknown population of X-ray sources in the inner arms of the Galaxy. IGR J17544-2619, IGR J16465-4507 and XTE J1739-302 are among these sources. Although the nature of these systems is still unexplained, the investigations of the optical/NIR counterparts of the two last sources, combined with high energy data, have provided evidence of them being highly absorbed high mass X-ray binaries with blue supergiant secondaries and displaying fast X-ray transient behaviour. In this work we present our optical/NIR observations of IGR J17544-2619, aimed at identifying and characterizing its counterpart. We show that the source is a high mass X-ray binary at a distance of 2-4 kpc with a strongly absorbed O9Ib secondary, and discuss the nature of the system.
Fil: Pellizza González, Leonardo Javier. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Universite Paris Diderot - Paris 7; Francia
Fil: Chaty, S.. Universite Paris Diderot - Paris 7; Francia
Fil: Negueruela, I.. Universidad de Alicante; España
description One of the most recent discoveries of the INTEGRAL observatory is the existence of a previously unknown population of X-ray sources in the inner arms of the Galaxy. IGR J17544-2619, IGR J16465-4507 and XTE J1739-302 are among these sources. Although the nature of these systems is still unexplained, the investigations of the optical/NIR counterparts of the two last sources, combined with high energy data, have provided evidence of them being highly absorbed high mass X-ray binaries with blue supergiant secondaries and displaying fast X-ray transient behaviour. In this work we present our optical/NIR observations of IGR J17544-2619, aimed at identifying and characterizing its counterpart. We show that the source is a high mass X-ray binary at a distance of 2-4 kpc with a strongly absorbed O9Ib secondary, and discuss the nature of the system.
publishDate 2006
dc.date.none.fl_str_mv 2006-08
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/11336/16672
Pellizza González, Leonardo Javier; Chaty, S.; Negueruela, I.; IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations; Edp Sciences; Astronomy And Astrophysics; 455; 2; 8-2006; 653-658
0004-6361
url http://hdl.handle.net/11336/16672
identifier_str_mv Pellizza González, Leonardo Javier; Chaty, S.; Negueruela, I.; IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations; Edp Sciences; Astronomy And Astrophysics; 455; 2; 8-2006; 653-658
0004-6361
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20054436
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2006/32/aa4436-05/aa4436-05.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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