The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643
- Autores
- Combi, Jorge Ariel; Ribó, Marc; Mirabel Miquele, Igor Felix; Sugizaki, Mutsumi
- Año de publicación
- 2004
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present a multiwavelength study of the field containing the unidentified X-ray source AX J1639.0-4642, discovered with the ASCA observatory and recently detected with the IBIS telescope, onboard the INTEGRAL satellite, dubbed IGR J16393-4643. The huge hydrogen column density towards the source, the hard spectral index in the 0.7-10 keV band and its flux variability suggest that the source is a High Mass X-ray Binary (HMXB) enshrouded by dust. Our search reveals the presence of a non-thermal radio counterpart within the X-ray error box. After a study of the broadband emission from X-rays to the radio domain, we propose that AX J1639.0-4642 is a dust-enshrouded Microquasar (MQ) candidate. In addition, the X-ray source is well within the 95% location contour of the unidentified γ-ray source 3EG J1639-4702. The main properties of AX J1639.0-4642/3EG J1639-4702 are consistent with those of two other MQs previously proposed to display high-energy γ-ray emission.
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: Ribó, Marc. Universidad de Barcelona; España
Fil: Mirabel Miquele, Igor Felix. Centre D; Francia
Fil: Sugizaki, Mutsumi. University of California; Estados Unidos - Materia
-
Stars
Binary stars
Radio continuum
Gamma ray observations - 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:11336/29898
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oai:ri.conicet.gov.ar:11336/29898 |
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The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643Combi, Jorge ArielRibó, MarcMirabel Miquele, Igor FelixSugizaki, MutsumiStarsBinary starsRadio continuumGamma ray observationshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a multiwavelength study of the field containing the unidentified X-ray source AX J1639.0-4642, discovered with the ASCA observatory and recently detected with the IBIS telescope, onboard the INTEGRAL satellite, dubbed IGR J16393-4643. The huge hydrogen column density towards the source, the hard spectral index in the 0.7-10 keV band and its flux variability suggest that the source is a High Mass X-ray Binary (HMXB) enshrouded by dust. Our search reveals the presence of a non-thermal radio counterpart within the X-ray error box. After a study of the broadband emission from X-rays to the radio domain, we propose that AX J1639.0-4642 is a dust-enshrouded Microquasar (MQ) candidate. In addition, the X-ray source is well within the 95% location contour of the unidentified γ-ray source 3EG J1639-4702. The main properties of AX J1639.0-4642/3EG J1639-4702 are consistent with those of two other MQs previously proposed to display high-energy γ-ray emission.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; ArgentinaFil: Ribó, Marc. Universidad de Barcelona; EspañaFil: Mirabel Miquele, Igor Felix. Centre D; FranciaFil: Sugizaki, Mutsumi. University of California; Estados UnidosEDP Sciences2004-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/29898Combi, Jorge Ariel; Ribó, Marc; Mirabel Miquele, Igor Felix; Sugizaki, Mutsumi; The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643; EDP Sciences; Astronomy and Astrophysics; 422; 8-2004; 1031-10370004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20047175info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2004/30/aa0175-04/aa0175-04.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 Técnicas2025-09-29T10:43:55Zoai:ri.conicet.gov.ar:11336/29898instacron: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 10:43:55.68CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643 |
title |
The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643 |
spellingShingle |
The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643 Combi, Jorge Ariel Stars Binary stars Radio continuum Gamma ray observations |
title_short |
The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643 |
title_full |
The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643 |
title_fullStr |
The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643 |
title_full_unstemmed |
The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643 |
title_sort |
The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643 |
dc.creator.none.fl_str_mv |
Combi, Jorge Ariel Ribó, Marc Mirabel Miquele, Igor Felix Sugizaki, Mutsumi |
author |
Combi, Jorge Ariel |
author_facet |
Combi, Jorge Ariel Ribó, Marc Mirabel Miquele, Igor Felix Sugizaki, Mutsumi |
author_role |
author |
author2 |
Ribó, Marc Mirabel Miquele, Igor Felix Sugizaki, Mutsumi |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
Stars Binary stars Radio continuum Gamma ray observations |
topic |
Stars Binary stars Radio continuum Gamma ray observations |
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 present a multiwavelength study of the field containing the unidentified X-ray source AX J1639.0-4642, discovered with the ASCA observatory and recently detected with the IBIS telescope, onboard the INTEGRAL satellite, dubbed IGR J16393-4643. The huge hydrogen column density towards the source, the hard spectral index in the 0.7-10 keV band and its flux variability suggest that the source is a High Mass X-ray Binary (HMXB) enshrouded by dust. Our search reveals the presence of a non-thermal radio counterpart within the X-ray error box. After a study of the broadband emission from X-rays to the radio domain, we propose that AX J1639.0-4642 is a dust-enshrouded Microquasar (MQ) candidate. In addition, the X-ray source is well within the 95% location contour of the unidentified γ-ray source 3EG J1639-4702. The main properties of AX J1639.0-4642/3EG J1639-4702 are consistent with those of two other MQs previously proposed to display high-energy γ-ray emission. 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: Ribó, Marc. Universidad de Barcelona; España Fil: Mirabel Miquele, Igor Felix. Centre D; Francia Fil: Sugizaki, Mutsumi. University of California; Estados Unidos |
description |
We present a multiwavelength study of the field containing the unidentified X-ray source AX J1639.0-4642, discovered with the ASCA observatory and recently detected with the IBIS telescope, onboard the INTEGRAL satellite, dubbed IGR J16393-4643. The huge hydrogen column density towards the source, the hard spectral index in the 0.7-10 keV band and its flux variability suggest that the source is a High Mass X-ray Binary (HMXB) enshrouded by dust. Our search reveals the presence of a non-thermal radio counterpart within the X-ray error box. After a study of the broadband emission from X-rays to the radio domain, we propose that AX J1639.0-4642 is a dust-enshrouded Microquasar (MQ) candidate. In addition, the X-ray source is well within the 95% location contour of the unidentified γ-ray source 3EG J1639-4702. The main properties of AX J1639.0-4642/3EG J1639-4702 are consistent with those of two other MQs previously proposed to display high-energy γ-ray emission. |
publishDate |
2004 |
dc.date.none.fl_str_mv |
2004-08 |
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/11336/29898 Combi, Jorge Ariel; Ribó, Marc; Mirabel Miquele, Igor Felix; Sugizaki, Mutsumi; The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643; EDP Sciences; Astronomy and Astrophysics; 422; 8-2004; 1031-1037 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/29898 |
identifier_str_mv |
Combi, Jorge Ariel; Ribó, Marc; Mirabel Miquele, Igor Felix; Sugizaki, Mutsumi; The dust-enshrouded microquasar candidate AX J1639.0-4642 = IGR J16393-4643; EDP Sciences; Astronomy and Astrophysics; 422; 8-2004; 1031-1037 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/10.1051/0004-6361:20047175 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2004/30/aa0175-04/aa0175-04.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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1844614475154456576 |
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13.070432 |