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Modelling steep radial emissivity in relativistic iron lines from black-hole accretion discs

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    0450994 - ASÚ 2016 RIV CZ eng C - Conference Paper (international conference)
    Svoboda, Jiří - Dovčiak, Michal - Karas, Vladimír - Goosmann, R. W.
    Modelling steep radial emissivity in relativistic iron lines from black-hole accretion discs.
    Proceedings of RAGtime 10/13: Workshops on black holes and neutron stars. Opava: Silesian University, 2014 - (Stuchlík, Z.), s. 209-221. Publications of the Institute of Physics, 6. ISBN 9788075101242. ISSN 2336-5668.
    [RAGtime /10.-13./. Opava (CZ), 15.09.2008-17.09.2008]
    R&D Projects: GA ČR(CZ) GP14-20970P
    Institutional support: RVO:67985815
    Keywords : black holes * accretion discs * relativistic iron lines
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

    The authors discuss whether the special conditions on the corona properties are indeed required, and/or whether the steep radial emissivity could be an artefact of model assumptions.
    Permanent Link: http://hdl.handle.net/11104/0252241

     
     
Number of the records: 1  

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