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Understanding the iron K alpha line emissivity profile with GR radiative transfer code

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00539460" target="_blank" >RIV/67985815:_____/20:00539460 - isvavai.cz</a>

  • Result on the web

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Understanding the iron K alpha line emissivity profile with GR radiative transfer code

  • Original language description

    In this work, we present calculations of the illumination and the iron K alpha emissivity profiles performed with the GR radiative transfer code Monk that employs the Monte Carlo method. In most previous studies the distinction between the illumination and emissivity profiles was not clearly made. For AGN discs, the emissivity profile has a similar shape with the illumination profile, but in the inner most region the former is steeper than the latter, where as for accretion discs in black hole X-ray binaries, the distinction between the two profiles is more dramatic. We find out that the different behavior between AGN and black hole X-ray binary discs is due to the different energy spectra of the illuminating radiation. This suggests that the emissivity profile of the iron Kαline cannot be determined by black hole spin and corona geometry alone and the energy spectrum of the illuminating radiation has to be taken into account. We also study the dependence of the emissivity profile on the geometry of the corona.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA17-02430S" target="_blank" >GA17-02430S: Geometrical properties of the accretion disc corona in Active Galactic Nuclei</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2020

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    Proceedings of RAGtime 20/22: Workshops on black holes and neutron stars

  • ISBN

    978-80-7510-433-5

  • ISSN

    2336-5676

  • e-ISSN

    2336-5676

  • Number of pages

    14

  • Pages from-to

    383-396

  • Publisher name

    Silesian University

  • Place of publication

    Opava

  • Event location

    Opava

  • Event date

    Oct 15, 2018

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article