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It is expected that extreme mass accretion rate onto strongly magnetised neutron star results in appearance of accretion columns above stellar surface. For a distant observer, rotation of a star results in periodic variations of X-ray flux. Because t
Externí odkaz:
http://arxiv.org/abs/2404.04137
Publikováno v:
Monthly Notices of the Royal Astronomical Society; May2024, Vol. 530 Issue 3, p3051-3058, 8p
