Abstract The results of X-ray and photometric observations (1981–1987) are given for the Be star X-ray binary A 0535+26. An analysis of the photometric and X-ray data enabled us to determine the radiation of a disk of accreting matter that gradually accumulates, precipitating afterwards on the neutron star's surface. The latter causes an X-ray flare. Physical parameters of the accreting accumulating disk are determined.


    Access

    Check access

    Check availability in my library

    Order at Subito €


    Export, share and cite



    Title :

    Optical and infrared radiation from accretion disks in be star X-ray binaries


    Contributors:
    Gnedin, Y. (author) / Larionov, V. (author) / Liutyi, V. (author) / Zaytzeva, G. (author)

    Published in:

    Advances in Space Research ; 8 , 2-3 ; 157-161


    Publication date :

    1988-01-01


    Size :

    5 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



    Accretion disks in bright X-ray binaries

    Inoue, H. | British Library Online Contents | 1993


    Turbulent Comptonization in relativistic accretion disks

    Socrates, A. / Davis, S. W. / Blaes, O. et al. | British Library Conference Proceedings | 2006



    Magnetohydrodynamic Simulations of Accretion Disks Around a Weakly Magnetized Neutron Star in Strong Gravity

    Kato, Y. / Hayashi, M. R. / Miyaji, S. et al. | British Library Conference Proceedings | 2001


    Accretion-disc radius variations in close binaries

    Hameury, J. M. / Lasota, J. P. / COSPAR | British Library Conference Proceedings | 2006