Obscured sources and Supergiant Fast X-ray Transients: new classes of high mass X-ray binaries
Abstract
A new type of high-energy binary systems has been revealed by the INTEGRAL satellite. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared observations. Among these sources, two distinct classes are appearing: the first one is constituted of intrinsically obscured high-energy sources, of which IGR J16318-4848 seems to be the most extreme example. The second one is populated by the so-called supergiant fast X-ray transients, with IGR J17544-2619 being the archetype. We report here on multi-wavelength optical to mid-infrared observations of a sample of 21 INTEGRAL sources. We show that in the case of the obscured sources our observations suggest the presence of absorbing material (dust and/or cold gas) enshrouding the whole binary system. We finally discuss the nature of these two different types of sources, in the context of high energy binary systems.
Keywords
Cite
@article{arxiv.0710.0292,
title = {Obscured sources and Supergiant Fast X-ray Transients: new classes of high mass X-ray binaries},
author = {Sylvain Chaty},
journal= {arXiv preprint arXiv:0710.0292},
year = {2007}
}
Comments
Invited talk at the Frascati Workshop 2007, Vulcano, Italy, May 28 - June 2; Multifrequency Behaviour of High Energy Cosmic Sources. 6 pages, 2 figures, 1 table