Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. II. The environment of the companion star

Abstract

Context: The INTEGRAL mission has led to the discovery of a new type of supergiant X-ray binaries (SGXBs), whose physical properties differ from those of previously known SGXBs. Those sources are in the course of being unveiled by means of multi-wavelength X-rays, optical, near- and mid-infrared observations, and two classes are appearing. The first class consists of obscured persistent SGXBs and the second is populated by the so-called supergiant fast X-ray transients (SFXTs). Aims: We report here mid-infrared (MIR) observations of the companion stars of twelve SGXBs from these two classes in order to assess the contribution of the star and the material enshrouding the system to the total emission.} Methods: We used data from observations we carried out at ESO/VLT with VISIR, as well as archival and published data, to perform broad-band spectral energy distributions of the companion stars and fitted them with a combination of two black bodies representing the star and a MIR excess due to the absorbing material enshrouding the star, if there was any. Results: We detect a MIR excess in the emission of IGR J16318-4848, IGR J16358-4726, and perhaps IGR J16195-4945. The other sources do not exhibit any MIR excess even when the intrinsic absorption is very high. (abridged)

A&A in press, The official date of acceptance is 25/01/2008, 17 pages, 4 figures, 9 tables. New version with english language editing required by editor, note added in proof

References in corpus (5)

• The 3rd IBIS/ISGRI soft gamma-ray survey catalog
• Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. I. The nature of the companion star
• A description of sources detected by INTEGRAL during the first 4 years of observations
• A search for counterparts to massive X-ray binaries using photometric catalogues
• The Rich Mid-Infrared Environments of Two Highly-Obscured X-ray Binaries: Spitzer Observations of IGR J16318-4848 and GX 301-2

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• Monitoring Supergiant Fast X-ray Transients with Swift. Results from the first year
• IGR J18483-0311: a new intermediate supergiant fast X-ray transient
• IGRJ16479-4514: the first eclipsing supergiant fast X-ray transient?
• Swift follow-up observations of 17 INTEGRAL sources of uncertain or unknown nature