Unveiling the nature of IGR J17497-2821 using X-ray and near-infrared observations

A. Paizis; M. A. Nowak; S. Chaty; J. Rodriguez; T. J.L. Courvoisier; M. Del Santo; K. Ebisawa; R. Farinelli; P. Ubertini; J. Wilms

doi:10.1086/513313

Unveiling the nature of IGR J17497-2821 using X-ray and near-infrared observations

A. Paizis
, M. A. Nowak
, S. Chaty
, J. Rodriguez
, T. J.L. Courvoisier
, M. Del Santo
, K. Ebisawa
, R. Farinelli
, P. Ubertini
, J. Wilms

INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
Massachusetts Institute of Technology
Université Paris-Diderot
University of Geneva
Université de Genève
INAF-IASF
ISAS/JAXA
University of Ferrara
Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen

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

10 Citations (Scopus)

Résumé

We report on a Chandra grating observation of the recently discovered hard X-ray transient IGR J17497-2821. The observation took place about 2 weeks after the discovery of the source at a flux level of about 20 mcrab in the 0.8-8 keV range. We extracted the most precise X-ray position of IGR J17497-2821, i.e., α_J2000 = 17^h49^m38.037^s, δ_J2000 = -28°21′17.37″ (with a 90% uncertainty of 0.6″). We also report on optical and near-infrared photometric follow-up observations based on this position. With the multiwavelength information at hand, we discuss the possible nature of the source, proposing that IGR J17497-2821 is a low-mass X-ray binary, most likely hosting a black hole, with a red giant K-type companion.

langue originale	Anglais
Pages (de - à)	L109-L112
journal	Astrophysical Journal
Volume	657
Numéro de publication	2 II
Les DOIs	https://doi.org/10.1086/513313
état	Publié - 10 mars 2007
Modification externe	Oui

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@article{408d93d501954994ad2de3cfd4b650f8,

title = "Unveiling the nature of IGR J17497-2821 using X-ray and near-infrared observations",

abstract = "We report on a Chandra grating observation of the recently discovered hard X-ray transient IGR J17497-2821. The observation took place about 2 weeks after the discovery of the source at a flux level of about 20 mcrab in the 0.8-8 keV range. We extracted the most precise X-ray position of IGR J17497-2821, i.e., αJ2000 = 17h49m38.037s, δJ2000 = -28°21′17.37″ (with a 90\% uncertainty of 0.6″). We also report on optical and near-infrared photometric follow-up observations based on this position. With the multiwavelength information at hand, we discuss the possible nature of the source, proposing that IGR J17497-2821 is a low-mass X-ray binary, most likely hosting a black hole, with a red giant K-type companion.",

keywords = "Binaries: close, Stars: individual (IGR J17497-2821), X-rays: binaries",

author = "A. Paizis and Nowak, \{M. A.\} and S. Chaty and J. Rodriguez and Courvoisier, \{T. J.L.\} and \{Del Santo\}, M. and K. Ebisawa and R. Farinelli and P. Ubertini and J. Wilms",

year = "2007",

month = mar,

day = "10",

doi = "10.1086/513313",

language = "English",

volume = "657",

pages = "L109--L112",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

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TY - JOUR

T1 - Unveiling the nature of IGR J17497-2821 using X-ray and near-infrared observations

AU - Paizis, A.

AU - Nowak, M. A.

AU - Chaty, S.

AU - Rodriguez, J.

AU - Courvoisier, T. J.L.

AU - Del Santo, M.

AU - Ebisawa, K.

AU - Farinelli, R.

AU - Ubertini, P.

AU - Wilms, J.

PY - 2007/3/10

Y1 - 2007/3/10

N2 - We report on a Chandra grating observation of the recently discovered hard X-ray transient IGR J17497-2821. The observation took place about 2 weeks after the discovery of the source at a flux level of about 20 mcrab in the 0.8-8 keV range. We extracted the most precise X-ray position of IGR J17497-2821, i.e., αJ2000 = 17h49m38.037s, δJ2000 = -28°21′17.37″ (with a 90% uncertainty of 0.6″). We also report on optical and near-infrared photometric follow-up observations based on this position. With the multiwavelength information at hand, we discuss the possible nature of the source, proposing that IGR J17497-2821 is a low-mass X-ray binary, most likely hosting a black hole, with a red giant K-type companion.

AB - We report on a Chandra grating observation of the recently discovered hard X-ray transient IGR J17497-2821. The observation took place about 2 weeks after the discovery of the source at a flux level of about 20 mcrab in the 0.8-8 keV range. We extracted the most precise X-ray position of IGR J17497-2821, i.e., αJ2000 = 17h49m38.037s, δJ2000 = -28°21′17.37″ (with a 90% uncertainty of 0.6″). We also report on optical and near-infrared photometric follow-up observations based on this position. With the multiwavelength information at hand, we discuss the possible nature of the source, proposing that IGR J17497-2821 is a low-mass X-ray binary, most likely hosting a black hole, with a red giant K-type companion.

KW - Binaries: close

KW - Stars: individual (IGR J17497-2821)

KW - X-rays: binaries

U2 - 10.1086/513313

DO - 10.1086/513313

M3 - Article

AN - SCOPUS:33947681121

SN - 0004-637X

VL - 657

SP - L109-L112

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2 II

ER -

Unveiling the nature of IGR J17497-2821 using X-ray and near-infrared observations

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