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Beyond the standard model of the disc-line spectral profiles from black hole accretion discs

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00442447" target="_blank" >RIV/67985815:_____/14:00442447 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.14311/AP.2014.54.0301" target="_blank" >http://dx.doi.org/10.14311/AP.2014.54.0301</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.14311/AP.2014.54.0301" target="_blank" >10.14311/AP.2014.54.0301</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Beyond the standard model of the disc-line spectral profiles from black hole accretion discs

  • Original language description

    The strong gravitational field of a black hole has distinct effects on the observed profile of a spectral line from an accretion disc near a black hole. The observed profile of the spectral line is broadened and skewed by a fast orbital motion and redshifted by a gravitational field. These effects can help us to constrain the parameters of a system with a black hole, both in active galactic nuclei and in a stellar-mass black hole. Here we explore the fact that an accretion disc emission can be mathematically imagined as a superposition of radiating accretion rings that extend from the inner edge to the outer rim of the disc, with some radially varying emissivity. In our work, we show that a characteristic double-horn profile of several radially confined (relatively narrow) accretion rings or belts could be recognized by the planned instruments onboard future satellites (such as the proposed ESA Large Observatory for X-ray Timing).

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GC13-00070J" target="_blank" >GC13-00070J: Accretion process in strong gravity of Galactic Center</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2014

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Acta polytechnica

  • ISSN

    1210-2709

  • e-ISSN

  • Volume of the periodical

    54

  • Issue of the periodical within the volume

    4

  • Country of publishing house

    CZ - CZECH REPUBLIC

  • Number of pages

    4

  • Pages from-to

    301-304

  • UT code for WoS article

  • EID of the result in the Scopus database