X-ray Lines in Binary Star Systems and the 3.55-keV Anomaly |
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Authors: | Burdyuzha V. V. |
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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... |
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