With the observational data of the Hard X-ray Modulation Telescope (HXMT), the first X-ray astronomical satellite of China, Dr. Ding Guoqiang from the Xinjiang Astronomical Observatory of the Chinese Academy of Sciences, along with his collaborators, investigated the hard X-ray tail of neutron star low-mass X-ray binaries (NS-LMXBs). Their results were published in The Astrophysical Journal on June 12.
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Source: Phys.org