Black hole accretion disk models at moderately high accretion rates have been constructed, taking correctly into account dissipation and heat transport in the transonic part of the flow. The present models differ from those of Shakura and Sunyaev (1973) in many important respects. The surface density at a given radius relates to the accretion rate through an S-shaped function.


    Zugriff

    Zugriff über TIB

    Verfügbarkeit in meiner Bibliothek prüfen


    Exportieren, teilen und zitieren



    Titel :

    Slim accretion disks around black holes


    Beteiligte:
    Szuszkiewicz, E. (Autor:in) / Czerny, B. (Autor:in) / Abramowicz, M. A. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1988-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Slim accretion disks around black holes

    Szuszkiewicz, E. / Czerny, B. / Abramowicz, M.A. | Elsevier | 1988



    Relativistic emission lines from accretion disks around black holes

    Čadež, Andrej / Calvani, Massimo | Elsevier | 2005


    Light curves and hard radiation anisotropy of accretion disks around black holes in LMC X-3 and A 0620-00

    Khruzina, T.S. / Cherepaschuk, A.M. / Shakura, N.I. et al. | Elsevier | 1988


    Hydrodynamics of Accretion onto Black Holes

    Park, M.-G. / Ostriker, J. P. / COSPAR; Scientific Commission E | British Library Conference Proceedings | 1998