IGR J18293-1213 is an eclipsing Cataclysmic Variable
arXiv:1605.08802 · doi:10.1093/mnras/stw1330
Abstract
Studying the population of faint hard X-ray sources along the plane of the Galaxy is challenging because of high-extinction and crowding, which make the identification of individual sources more difficult. IGR J18293-1213 is part of the population of persistent sources which have been discovered by the INTEGRAL satellite. We report on NuSTAR and Swift/XRT observations of this source, performed on 2015 September 11. We detected three eclipsing intervals in the NuSTAR light curve, allowing us to constrain the duration of these eclipses, min, and the orbital period of the system, hr. Even though we only report an upper limit on the amplitude of a putative spin modulation, the orbital period and the hard thermal Bremsstrahlung spectrum of IGR J18293-1213 provide strong evidence that this source is a magnetic Cataclysmic Variable (CV). Our NuSTAR and Swift/XRT joint spectral analysis places strong constraints on the white dwarf mass M. Assuming that the mass to radius ratio of the companion star (solar units) and using , and , we derived the mass of the companion star M, the orbital separation of the binary system R, and its orbital inclination compared to the line of sight .
8 pages, 5 figures, accepted for publication in MNRAS
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