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5 ta ish

Ish: THE RELATIVISTIC IRON Kα LINE FROM AN ACCRETION DISC ONTO A STATIC NON-BARYONIC COMPACT OBJECT

  1. Testing the Kerr Black Hole Hypothesis with GX 339–4 by a Combined Analysis of Its Thermal Spectrum and Reflection Features

    Ashutosh Tripathi, Askar B. Abdikamalov, Dimitry Ayzenberg +3

    MaqolaAstrophysical Phenomena and ObservationsThe Astrophysical Journal202123 iqtibos
    ABI

  2. 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

    MaqolaAstrophysical Phenomena and ObservationsThe Astrophysical Journal202217 iqtibos
    ABI

  3. Testing the Kerr black hole hypothesis with the continuum-fitting and the iron line methods: the case of GRS 1915+105

    Ashutosh Tripathi, Askar B. Abdikamalov, Dimitry Ayzenberg +4

    MaqolaAstrophysical Phenomena and ObservationsJournal of Cosmology and Astroparticle Physics202214 iqtibos
    ABI

  4. Testing the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>δ</mml:mi></mml:math>-Kerr metric with black hole x-ray data

    J Tao, Shafqat Riaz, Biao Zhou +3

    MaqolaAstrophysical Phenomena and ObservationsPhysical review. D/Physical review. D.20234 iqtibos
    ABI

  5. Constraining the Konoplya-Rezzolla-Zhidenko deformation parameters. II. Limits from stellar-mass black hole x-ray data

    Zhibo Yu, Qunfeng Jiang, Askar B. Abdikamalov +5

    MaqolaAstrophysical Phenomena and ObservationsPhysical review. D/Physical review. D.20213 iqtibos
    ABI