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Long-term observations of the Cyg X-3 and ??Cygni SNR at ultrahigh energies by SHALON mirror Cherenkov telescopesBULLETIN- LEBEDEV PHYSICS INSTITUTE C/C OF KRATKIE SOOBSHCHENIIA PO FIZIKESinitsinaV.G.V.Y.
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When re-emitting the optical component light, an oblique precessing accretion disk gives rise to a photometric variability with the first and higher harmonics of the precession period (the phase δ) and the period defined by the sum of/or the difference between, the frequencies of the orbital ...
Tylenda, RSpringer NetherlandsTylenda, R. (1977). The continuous radiation emitted by accretion discs in cataclysmic binaries - The dwarf nova SS CYG during outburst and the old novae V 603 AQL and RR PIC, Acta Astronomica 27: 235-249....
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