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      Permanent link:
      https://www.ias.ac.in/article/fulltext/joaa/023/01-02/0143-0147

    • Keywords

       

      Accretion; accretion disk; black hole physics; shock Waves; outflows

    • Abstract

       

      We self-consistently obtain shock locations in an accretion flow by using an analytical method. One can obtain the spectral properties, quasi-periodic oscillation frequencies and the outflow rates when the inflow parameters are known. Since temperature of the CENBOL decides the spectral states of the black hole, and also the outflow rate, the outflow rate is directly related to the spectral states.

    • Author Affiliations

       

      Santabrata Das1 Sandip K. Chakrabarti1

      1. S N Bose National Center for Basic Sciences, Block — JD; Sector — III, Salt Lake, Kolkata—98, West Bengal, India
    • Dates

       
  • Journal of Astrophysics and Astronomy | News

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      Posted on January 27, 2016

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