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Exploring the X-ray universe via timing: Mass of the active galactic nucleus black hole XMMUJ134736.6+173403

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19630%2F21%3AA0000173" target="_blank" >RIV/47813059:19630/21:A0000173 - isvavai.cz</a>

  • Result on the web

    <a href="https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/abs/exploring-the-xray-universe-via-timing-mass-of-the-active-galactic-nucleus-black-hole-xmmuj1347366173403/8F85460501CAA93C58B44284B65D8784" target="_blank" >https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/abs/exploring-the-xray-universe-via-timing-mass-of-the-active-galactic-nucleus-black-hole-xmmuj1347366173403/8F85460501CAA93C58B44284B65D8784</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1017/S1743921320003312" target="_blank" >10.1017/S1743921320003312</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Exploring the X-ray universe via timing: Mass of the active galactic nucleus black hole XMMUJ134736.6+173403

  • Original language description

    A strong quasi-periodic modulation has recently been revealed in the X-ray flux of the X-ray source XMMUJ134736.6+173403. The two observed twin-peak quasiperiodic oscillations (QPOs) exhibit a 3:1 frequency ratio and strongly support the evidence for the presence of an active galactic nucleus black hole (AGN BH). It has been suggested that detections of twin-peak QPOs with commensurable frequency ratios and scaling of their periods with BH mass could provide the basis for a method intended to determine the mass of BH sources, such as AGNs. Assuming the orbital origin of QPOs, we calculate the upper and lower limit on the AGN BH mass M, reaching M 107-109 M™. Compared to mass estimates of other sources, XMMUJ134736.6+173403 appears to be the most massive source with commensurable QPO frequencies, and its mass represents the current observational upper limit on the AGN BH mass obtained from the QPO observations.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2021

  • 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 the International Astronomical Union

  • ISBN

  • ISSN

    1743-9213

  • e-ISSN

    1743-9221

  • Number of pages

    12

  • Pages from-to

    348-350

  • Publisher name

    Cambridge University Press

  • Place of publication

    Cambridge

  • Event location

    Cambridge

  • Event date

    Jan 1, 2021

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article