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Predictions for the reverberating spectral line signal from a newly formed black hole accretion disk: case of tidal disruption flares

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00445289" target="_blank" >RIV/67985815:_____/15:00445289 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1088/0004-637X/807/1/89" target="_blank" >http://dx.doi.org/10.1088/0004-637X/807/1/89</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/0004-637X/807/1/89" target="_blank" >10.1088/0004-637X/807/1/89</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Predictions for the reverberating spectral line signal from a newly formed black hole accretion disk: case of tidal disruption flares

  • Original language description

    Tidal disruption events (TDEs) can be perfect probes of dormant supermassive black holes in normal galaxies. During the rising phase, the accretion luminosity can increase by orders of magnitude in several weeks, and the emergent ionizing radiation illuminates the fresh accretion flow. In this paper, we simulated the evolution of the expected spectral line profile of iron due to such a flare by using a ray-tracing code with effects of general relativity taken into account. We found that the time-dependent profile changes significantly with black hole spin, inclination angle with respect to the black hole equatorial plane, and the expansion velocity of the ionization front. At low values of spin, a ?loop feature appears in the line profile versus time plot when the inclination is no less than 30° and the expansion velocity vexp is no less than half the speed of light, owing to a shadow in the emission of the truncated disk. Our results demonstrate the importance of searching for X-ray s

  • 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

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2015

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astrophysical Journal

  • ISSN

    0004-637X

  • e-ISSN

  • Volume of the periodical

    807

  • Issue of the periodical within the volume

    89

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    12

  • Pages from-to

    1-12

  • UT code for WoS article

    000358945200089

  • EID of the result in the Scopus database