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Super-massive black hole mass estimation from bright flares

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00567711" target="_blank" >RIV/67985815:_____/22:00567711 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1142/9789811258251_0113" target="_blank" >http://dx.doi.org/10.1142/9789811258251_0113</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1142/9789811258251_0113" target="_blank" >10.1142/9789811258251_0113</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Super-massive black hole mass estimation from bright flares

  • Original language description

    Super-Massive Black Holes reside in galactic nuclei, where they exhibit episodic bright flares due to accretion events. Taking into account relativistic effects, namely, the boosting and lensing of X-ray flares, we further examine the possibility to constraint the mass of the SMBH from the predicted profiles of the observed light curves. To this end, we have studied four bright flares from Sagittarius A*, which exhibit an asymmetric shape consistent with a combination of two intrinsically separate peaks that occur with a specific time delay with respect to each other. We have thus proposed (Karssen et al. 2017, Mon. Not. R. Astron. Soc. 472, 4422) that an interplay of relativistic effects could be responsible for the shape of the observed light curves and we tested the reliability of the method.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

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

    2022

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    The Fifteenth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories

  • ISBN

    978-981-125-825-1

  • ISSN

  • e-ISSN

  • Number of pages

    7

  • Pages from-to

    842-848

  • Publisher name

    World Scientific

  • Place of publication

    Singapore

  • Event location

    Rome

  • Event date

    Jul 1, 2018

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    001250440000109