http://arxiv.org/abs/2107.07215
Binary star systems represent a significant proportion of the Galactic stellar population, with X-ray binaries being an important subset of these for high energy astrophysics. Although hundreds of X-ray binaries are detected in the Milky Way and beyond, only 12 of these systems are listed in the 4FGL-DR2, the latest Fermi-LAT point source catalogue. With such a small number detectable by Fermi-LAT, much is still unknown about the mechanisms by which these systems emit $\gamma$-rays. We present the method and current status of our large-scale survey of the X-ray binary population using over 12 years of Fermi-LAT data, and current catalogues and background models.
M. Harvey, C. Rulten and P. Chadwick
Fri, 16 Jul 21
40/61
Comments: 8 pages, 1 figure, prepared for the Proceedings of the 37th International Cosmic Ray Conference (ICRC 2021)
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