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.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

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


    Beteiligte:
    Gnedin, Y. (Autor:in) / Larionov, V. (Autor:in) / Liutyi, V. (Autor:in) / Zaytzeva, G. (Autor:in)

    Erschienen in:

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


    Erscheinungsdatum :

    01.01.1988


    Format / Umfang :

    5 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



    Accretion disks in bright X-ray binaries

    Inoue, H. | British Library Online Contents | 1993


    Accretion-disc radius variations in close binaries

    Hameury, Jean-Marie | Online Contents | 2006


    Turbulent Comptonization in relativistic accretion disks

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


    Spiral Alfven instability in accretion disks

    Tagger, M. / Saclay, C. E. | British Library Online Contents | 1993