Abstract This paper suggests numerical model for accretion disc around neutron star of strong magnetic field in close binary system. The accretion disc is build up by constant external flux from secondary component. Conditions of magnetospheric “inclusion”, “exclussion” are imposed in aagreement which the analitical model of X-ray luminosity of such system is obtained for different velocities of disc accretion. The value of Mcr i.e. the minimum admissible accretion velocity balanced by magnetic field affects significantly the evolution type.


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    Titel :

    Numerical model of X-ray transient


    Beteiligte:
    Georgieva, E. (Autor:in) / Filipov, L. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 8 , 2-3 ; 493-496


    Erscheinungsdatum :

    1988-01-01


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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