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arXiv · 0704.3682

IGR J16194-2810: a new symbiotic X-ray binary

N. Masetti·R. Landi·M. L. Pretorius·V. Sguera·A. J. Bird·M. Perri·P. A. Charles·J. A. Kennea·A. Malizia·P. Ubertini
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Abstract

We here report on the multiwavelength study which led us to the identification of X-ray source IGR J16194-2810 as a new Symbiotic X-ray Binary (SyXB), that is, a rare type of Low Mass X-ray Binary (LMXB) composed of a M-type giant and a compact object. Using the accurate X-ray position allowed by Swift/XRT data, we pinpointed the optical counterpart, a M2 III star. Besides, the combined use of the spectral information afforded by XRT and INTEGRAL/IBIS shows that the 0.5-200 keV spectrum of this source can be described with an absorbed Comptonization model, usually found in LMXBs and, in particular, in SyXBs. No long-term (days to months) periodicities are detected in the IBIS data. The time coverage afforded by XRT reveals shot-noise variability typical of accreting Galactic X-ray sources, but is not good enough to explore the presence of X-ray short-term (seconds to hours) oscillations in detail. By using the above information, we infer important parameters for this source such as its distance (about 3.7 kpc) and X-ray luminosity (about 1.4e35 erg/s in the 0.5-200 keV band), and we give a description for this system (typical of SyXBs) in which a compact object (possibly a neutron star) accretes from the wind of its M-type giant companion. We also draw some comparisons between IGR J16194-2810 and other sources belonging to this subclass, finding that this object resembles SyXBs 4U 1700+24 and 4U 1954+31.

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N. Masetti, R. Landi, M. L. Pretorius, V. Sguera, A. J. Bird, M. Perri, P. A. Charles, J. A. Kennea, A. Malizia, P. Ubertini. 2007-06-22. IGR J16194-2810: a new symbiotic X-ray binary. https://doi.org/10.1051/0004-6361:20077509

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