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Иш: DEPENDENCE OF INNER ACCRETION DISK STRESS ON PARAMETERS: THE SCHWARZSCHILD CASE

  1. Testing the Kerr Black Hole Hypothesis with GRS 1716-249 by Combining the Continuum Fitting and the Iron-line Methods

    Zuobin Zhang, H. Liu, Askar B. Abdikamalov +3

    МақолаAstrophysical Phenomena and ObservationsThe Astrophysical Journal202217 иқтибос
    ABI

  2. Testing Relativistic Reflection Models with GRMHD Simulations of Accreting Black Holes

    Swarnim Shashank, Shafqat Riaz, Askar B. Abdikamalov +1

    МақолаAstrophysical Phenomena and ObservationsThe Astrophysical Journal20229 иқтибос
    ABI

  3. Probing the near-horizon region of Cygnus X-1 with <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>S</mml:mi><mml:mi>u</mml:mi><mml:mi>z</mml:mi><mml:mi>a</mml:mi><mml:mi>k</mml:mi><mml:mi>u</mml:mi></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>N</mml:mi><mml:mi>u</mml:mi><mml:mi>S</mml:mi><mml:mi>T</mml:mi><mml:mi>A</mml:mi><mml:mi>R</mml:mi></mml:math>

    Zuobin Zhang, H. Liu, Askar B. Abdikamalov +3

    МақолаAstrophysical Phenomena and ObservationsPhysical review. D/Physical review. D.20212 иқтибос
    ABI