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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/16672
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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 Técnicas2025-09-29T09:58:54Zoai: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:34982025-09-29 09:58:54.723CONICET 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 |
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reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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