Dataciencia

Colección SciELO Chile

Multi-frequency observations of Swift J1626.6-5156

Indexado

WoS	WOS:000295168100023
Scopus	SCOPUS_ID:80051970516

DOI

10.1051/0004-6361/201117301

Año

2011

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. The X-ray/optical/IR continuum and spectral features are typical of an accreting X-ray pulsar with an early-type donor. The long-term X-ray variability with its major and minor outbursts and quiescent emission is also characteristic of hard X-ray transients. We conclude that Swift J1626.6-5156 is a Be/X-ray binary with a B0Ve companion located at a distance of similar to 10 kpc.

Revista

Revista	ISSN
Astronomy & Astrophysics	1432-0746

Métricas Externas

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Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Reig, P.	Hombre	Fdn Res & Technol Hellas - Grecia Univ Crete - Grecia Foundation for Research and Technology-Hellas, Institute of Electronic Structure and Laser - Grecia Panepistimio Kritis - Grecia Institute of Electronic Structure and Laser of the Foundation for Research and Technology-Hellas - Grecia University of Crete - Grecia
2	Nespoli, E.	-	Univ Valencia - España Valencian Int Univ - España University of Valencia - España Universidad Internacional de Valencia - España Universitat de València - España
3	Fabregat, J.	Hombre	Univ Valencia - España University of Valencia - España Universitat de València - España
4	MENNICKENT-CID, RONALD ENRIQUE	Hombre	Universidad de Concepción - Chile Centro de Excelencia en Astrofísica y Tecnologías Afines - Chile

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Financiamiento

Fuente
FONDECYT
FEDER
European Regional Development Fund
COST Action
Generalitat Valenciana
Spanish Ministerio de Educación y Ciencia
Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica
BASAL Centro de Astrofisica y Tecnologias Afines (CATA)
Fondo Nacional de Desarrollo CientÃfico, TecnolÃ³gico y de InnovaciÃ³n TecnolÃ³gica
Centro de Astrofísica y Tecnologías Afines
Centro de AstrofÃsica y TecnologÃas Afines
Ministerio de Ciencia TecnologÃa y Telecomunicaciones
Chilean Center for Astrophysics
Ministerio de Educación Superior, Ciencia y Tecnología, República Dominicana

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Agradecimientos

Agradecimiento
We thank the referee, Malcolm Coe, for his useful and important comments that improved the final version of this manuscript. The work of E.N. y J.F. is supported by the Spanish Ministerio de Educacion y Ciencia, and FEDER, under contract AYA2010-18352. P.R. and J.F. are partially supported by the Generalitat Valenciana project of excellence PROMETEO/2009/064. PR also acknowledges partial support by the COST Action ECOST-STSM-MP0905-280611-008632. R.E.M. acknowledges support by Fondecyt grant 1070705, 1110347, the Chilean Center for Astrophysics FONDAP 15010003 and from the BASAL Centro de Astrofisica y Tecnologias Afines (CATA) PFB-06/2007. This work was based on observations collected at the European Southern Observatory, Chile (Programme ID: 085.D-0297A) and on data obtained from the ESO Science Archive Facility. This research has made use of the USNOFS Image and Catalogue Archive operated by the United States Naval Observatory, Flagstaff Station (http://www.nofs.navy.mil/data/fchpix/).
We thank the referee, Malcolm Coe, for his useful and important comments that improved the final version of this manuscript. The work of E.N. y J.F. is supported by the Spanish Ministerio de Educación y Ciencia, and FEDER, under contract AYA2010-18352. P.R. and J.F. are partially supported by the Generalitat Valenciana project of excellence PROMETEO/2009/064. PR also acknowledges partial support by the COST Action ECOST-STSM-MP0905-280611-008632. R.E.M. acknowledges support by Fondecyt grant 1070705, 1110347, the Chilean Center for Astrophysics FONDAP 15010003 and from the BASAL Centro de Astrofísica y Tecnologias Afines (CATA) PFB–06/2007. This work was based on observations collected at the European Southern Observatory, Chile (Programme ID: 085.D-0297A) and on data obtained from the ESO Science Archive Facility. This research has made use of the USNOFS Image and

Agradecimiento

We thank the referee, Malcolm Coe, for his useful and important comments that improved the final version of this manuscript. The work of E.N. y J.F. is supported by the Spanish Ministerio de Educacion y Ciencia, and FEDER, under contract AYA2010-18352. P.R. and J.F. are partially supported by the Generalitat Valenciana project of excellence PROMETEO/2009/064. PR also acknowledges partial support by the COST Action ECOST-STSM-MP0905-280611-008632. R.E.M. acknowledges support by Fondecyt grant 1070705, 1110347, the Chilean Center for Astrophysics FONDAP 15010003 and from the BASAL Centro de Astrofisica y Tecnologias Afines (CATA) PFB-06/2007. This work was based on observations collected at the European Southern Observatory, Chile (Programme ID: 085.D-0297A) and on data obtained from the ESO Science Archive Facility. This research has made use of the USNOFS Image and Catalogue Archive operated by the United States Naval Observatory, Flagstaff Station (http://www.nofs.navy.mil/data/fchpix/).

We thank the referee, Malcolm Coe, for his useful and important comments that improved the final version of this manuscript. The work of E.N. y J.F. is supported by the Spanish Ministerio de Educación y Ciencia, and FEDER, under contract AYA2010-18352. P.R. and J.F. are partially supported by the Generalitat Valenciana project of excellence PROMETEO/2009/064. PR also acknowledges partial support by the COST Action ECOST-STSM-MP0905-280611-008632. R.E.M. acknowledges support by Fondecyt grant 1070705, 1110347, the Chilean Center for Astrophysics FONDAP 15010003 and from the BASAL Centro de Astrofísica y Tecnologias Afines (CATA) PFB–06/2007. This work was based on observations collected at the European Southern Observatory, Chile (Programme ID: 085.D-0297A) and on data obtained from the ESO Science Archive Facility. This research has made use of the USNOFS Image and