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X-ray Lines in Binary Star Systems and the 3.55-keV Anomaly
Authors:Burdyuzha  V. V.
Affiliation:1.Astrospace Center, Lebedev Physical Institute, Russian Academy of Sciences, Profsoyuznaya ul. 84/32, 117997, Moscow, Russia
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Abstract:
Journal of Experimental and Theoretical Physics - A close binary star system that consists of a red giant and a neutron star is considered. X-ray emission from H-like Si XIV emerges during its...
Keywords:
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