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.


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    Titel :

    Analysis of V616 Mon/A 0620-00 brightness variations during the outburst of 1975–1976


    Beteiligte:
    Kurochkin, N.E. (Autor:in) / Bochkarev, N.G. (Autor:in) / Karitskaya, E.A. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 8 , 2-3 ; 227-235


    Erscheinungsdatum :

    1988-01-01


    Format / Umfang :

    9 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



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