Infrared identification of high-mass X-ray binaries discovered by INTEGRAL

@article{Coleiro2013InfraredIO,
  title={Infrared identification of high-mass X-ray binaries discovered by INTEGRAL},
  author={A. Coleiro and Sylvain Chaty and Juan Antonio Zurita Heras and Farid Rahoui and John A. Tomsick},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2013}
}
Since it started observing the sky, the INTEGRAL satellite has discovered new categories of high mass X-ray binaries (HMXB) in our Galaxy. These observations raise important questions on the formation and evolution of these rare and short-lived objects. We present here new infrared observations from which to reveal or constrain the nature of 15 INTEGRAL sources, which allow us to update and discuss the Galactic HMXB population statistics. After previous photometric and spectroscopic observing… 
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References

SHOWING 1-10 OF 76 REFERENCES
Unveiling the nature of INTEGRAL objects through optical spectroscopy VII. Identification of 20 Galactic and extragalactic hard X-ray sources
Within the framework of our program of assessment of the nature of unidentified or poorly known INTEGRAL sources, we present here spectroscopy of optical objects, selected through positional
Unveiling the nature of INTEGRAL objects through optical spectroscopy - VIII. Identification of 44 newly detected hard X-ray sources
(abridged) Hard X-ray surveys performed by the INTEGRAL satellite have discovered a conspicuous fraction (up to 30%) of unidentified objects among the detected sources. Here we continue our
BROADBAND ESO/VISIR-SPITZER INFRARED SPECTROSCOPY OF THE OBSCURED SUPERGIANT X-RAY BINARY IGR J16318-4848
A new class of X-ray binaries has been recently discovered by the high energy observatory, INTEGRAL. It is composed of intrinsically obscured supergiant high mass X-ray binaries, unveiled by means of
IGR J17544-2619: a new supergiant fast X-ray transient revealed by optical/infrared observations
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
Chandra Localizations and Spectra of INTEGRAL Sources in the Galactic Plane
We report on the results of observations of hard X-ray sources in the Galactic plane with the Chandra X-Ray Observatory. The hard X-ray IGR sources were discovered by the INTEGRAL satellite, and the
The soft X-ray counterpart of the newly discovered INTEGRAL source IGR J16195-4945
The INTEGRAL satellite, during its regular scanning observations of the Galactic plane, has discovered several new X-ray sources emitting above 20 keV. The nature of the great majority of them is
XMM-Newton and INTEGRAL observations of new absorbed supergiant high-mass X-ray binaries
Context. During the first year in operation, INTEGRAL, the European Space Agency’s γ-ray observatory, has detected more than 28 new bright sources in the galactic plane which emit the bulk of their
The optical/near-infrared counterpart of the integral obscured source IGR j16318-4848: An sgB[e] in a high-mass X-ray binary?
The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003 January 29. The high-energy spectrum exhibits such a high column density that the source is undetectable in X-rays
Unveiling the nature of INTEGRAL objects through optical spectroscopy. VI. A multi-observatory ident
Using 8 telescopes in the northern and southern hemispheres, plus archival data from two on-line sky surveys, we performed a systematic optical spectroscopic study of 39 putative counterparts of
The Swift-BAT survey reveals the orbital period of three high-mass X-ray binaries
Aims. A growing number of previously hidden Galactic X-ray sources are now detected with recent surveys performed by the INTEGRAL and Swift satellites. Most of these new sources eluded past surveys
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