Unveiling the nature of IGR J17177-3656 with X-ray, near-infrared, and radio observations

A. Paizis; M. A. Nowak; J. Wilms; S. Chaty; S. Corbel; J. Rodriguez; M. Del Santo; P. Ubertini; R. Chini

doi:10.1088/0004-637X/738/2/183

Unveiling the nature of IGR J17177-3656 with X-ray, near-infrared, and radio observations

A. Paizis
, M. A. Nowak
, J. Wilms
, S. Chaty
, S. Corbel
, J. Rodriguez
, M. Del Santo
, P. Ubertini
, R. Chini

INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
Massachusetts Institute of Technology
Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
Université Paris-Diderot
INAF-IASF
Ruhr-University Bochum
Universidad Católica del Norte

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

We report on the first broadband (1-200keV) simultaneous Chandra-INTEGRAL observations of the recently discovered hard X-ray transient IGR J17177-3656 that took place on 2011 March 22, about two weeks after the source discovery. The source had an average absorbed 1-200keV flux of about 8 × 10 ^-10 erg cm^-2 s^-1. We extracted a precise X-ray position of IGR J17177-3656, α_J2000 = 17^h17 ^m4262, δ_J2000 = -36°56′045 (90% uncertainty of 06). We also report Swift, near-infrared, and quasi-simultaneous radio follow-up observations. With the multi-wavelength information at hand, we propose IGR J17177-3656 is a low-mass X-ray binary, seen at high inclination, probably hosting a black hole.

langue originale	Anglais
Numéro d'article	183
journal	Astrophysical Journal
Volume	738
Numéro de publication	2
Les DOIs	https://doi.org/10.1088/0004-637X/738/2/183
état	Publié - 10 sept. 2011
Modification externe	Oui

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10.1088/0004-637X/738/2/183

Contient cette citation

@article{4d01ec8b1ee942aca53c218684d1fe0f,

title = "Unveiling the nature of IGR J17177-3656 with X-ray, near-infrared, and radio observations",

abstract = "We report on the first broadband (1-200keV) simultaneous Chandra-INTEGRAL observations of the recently discovered hard X-ray transient IGR J17177-3656 that took place on 2011 March 22, about two weeks after the source discovery. The source had an average absorbed 1-200keV flux of about 8 × 10 -10 erg cm-2 s-1. We extracted a precise X-ray position of IGR J17177-3656, αJ2000 = 17h17 m4262, δJ2000 = -36°56′045 (90\% uncertainty of 06). We also report Swift, near-infrared, and quasi-simultaneous radio follow-up observations. With the multi-wavelength information at hand, we propose IGR J17177-3656 is a low-mass X-ray binary, seen at high inclination, probably hosting a black hole.",

keywords = "X-rays: binaries, accretion, accretion disks, binaries: close, stars: individual (IGR J171773656)",

author = "A. Paizis and Nowak, \{M. A.\} and J. Wilms and S. Chaty and S. Corbel and J. Rodriguez and \{Del Santo\}, M. and P. Ubertini and R. Chini",

year = "2011",

month = sep,

day = "10",

doi = "10.1088/0004-637X/738/2/183",

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TY - JOUR

T1 - Unveiling the nature of IGR J17177-3656 with X-ray, near-infrared, and radio observations

AU - Paizis, A.

AU - Nowak, M. A.

AU - Wilms, J.

AU - Chaty, S.

AU - Corbel, S.

AU - Rodriguez, J.

AU - Del Santo, M.

AU - Ubertini, P.

AU - Chini, R.

PY - 2011/9/10

Y1 - 2011/9/10

N2 - We report on the first broadband (1-200keV) simultaneous Chandra-INTEGRAL observations of the recently discovered hard X-ray transient IGR J17177-3656 that took place on 2011 March 22, about two weeks after the source discovery. The source had an average absorbed 1-200keV flux of about 8 × 10 -10 erg cm-2 s-1. We extracted a precise X-ray position of IGR J17177-3656, αJ2000 = 17h17 m4262, δJ2000 = -36°56′045 (90% uncertainty of 06). We also report Swift, near-infrared, and quasi-simultaneous radio follow-up observations. With the multi-wavelength information at hand, we propose IGR J17177-3656 is a low-mass X-ray binary, seen at high inclination, probably hosting a black hole.

AB - We report on the first broadband (1-200keV) simultaneous Chandra-INTEGRAL observations of the recently discovered hard X-ray transient IGR J17177-3656 that took place on 2011 March 22, about two weeks after the source discovery. The source had an average absorbed 1-200keV flux of about 8 × 10 -10 erg cm-2 s-1. We extracted a precise X-ray position of IGR J17177-3656, αJ2000 = 17h17 m4262, δJ2000 = -36°56′045 (90% uncertainty of 06). We also report Swift, near-infrared, and quasi-simultaneous radio follow-up observations. With the multi-wavelength information at hand, we propose IGR J17177-3656 is a low-mass X-ray binary, seen at high inclination, probably hosting a black hole.

KW - X-rays: binaries

KW - accretion, accretion disks

KW - binaries: close

KW - stars: individual (IGR J171773656)

U2 - 10.1088/0004-637X/738/2/183

DO - 10.1088/0004-637X/738/2/183

M3 - Article

AN - SCOPUS:80052813654

SN - 0004-637X

VL - 738

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 183

ER -

Unveiling the nature of IGR J17177-3656 with X-ray, near-infrared, and radio observations

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