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- W2093349932 abstract "Analyzing the V616 Mon/A 0620-00 photoelectric observation data obtained during the decay phase of the 1975–1976 outburst has discriminated the brightness variations with the orbital period which is close to its present-day value. Besides, the period . Seems to have occured to one or another degree throughout the brightness decay interval. The decrease of brightness is mainly due to re - emission of a fading X - ray flux by accretion disk and by star. The light curve with is formed mainly due to X - ray flux re-emission by accretion disk and to mutual eclipses of the star and the disk. The possible variations of the orbital light curves with the brightness decay onset agree with the concept of a disk precessing with this period." @default.
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- W2093349932 date "1988-01-01" @default.
- W2093349932 modified "2023-09-25" @default.
- W2093349932 title "Analysis of V616 Mon/A 0620-00 brightness variations during the outburst of 1975–1976" @default.
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- W2093349932 doi "https://doi.org/10.1016/0273-1177(88)90412-7" @default.
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