The theory of radiation pressure supported thick accretion disks is discussed and observational evidence for their existence is reviewed. Theoretical aspects examined include luminosity, spectra, jets, and variability. Observational data of the binary system SS 433, compact X-ray sources (showing quasi-periodic oscillations), and active galactic nuclei are presented. The observed central masses, total luminosities, accretion rates, efficiencies, funnels, jets, and variabilities of objects thought to be thick accretion disks are given in a table and the history of the discovery of thick accretion disks is summarized.


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    Titel :

    Thick accretion disks ten years later


    Beteiligte:

    Erschienen in:

    Erscheinungsdatum :

    01.01.1988



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Thick accretion disks ten years later

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    Turbulent Comptonization in relativistic accretion disks

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


    Massive Accretion Disks in Galactic Nuclei

    Scoville, N.Z. | Online Contents | 1999