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.
Analysis of V616 Mon/A 0620-00 brightness variations during the outburst of 1975–1976
Advances in Space Research ; 8 , 2-3 ; 227-235
1988-01-01
9 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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