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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%2F67985815%3A_____%2F19%3A00518006" target="_blank" >RIV/67985815:_____/19:00518006 - isvavai.cz</a>

  • Result on the web

    <a href="http://hdl.handle.net/11104/0303224" target="_blank" >http://hdl.handle.net/11104/0303224</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201834774" target="_blank" >10.1051/0004-6361/201834774</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Mass of the active galactic nucleus black hole XMMUJ134736.6+173403

  • Original language description

    A recent study of the X-ray source XMMUJ134736.6+173403 has revealed a strong quasi-periodic modulation in the X-ray flux. The observation of two quasiperiodic oscillations (QPOs) that occur on a daily timescale and exhibit a 3:1 frequency ratio strongly supports the evidence for the presence of an active galactic nucleus black hole (AGN BH). Assuming an orbital origin of QPOs, we calculated the upper and lower limit on AGN BH mass M and found M approximate to 10(7)-10(9) M-circle dot. When we compare this 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 AGN BH mass based on QPO observations. We note that it will be crucial for the falsification of particular resonance models of QPOs whether only a single QPO with a frequency that completes the harmonic sequence 3:2:1 is found in this source, or if a new different pair of QPOs with frequencies in the 3: 2 ratio is found. The former case would agree with the prediction of the 3:2 epicyclic resonance model and BH mass M approximate to (5a(2) + 8a + 8) x 10(7) M-circle dot, where a is a dimensionless BH spin.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • 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

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2019

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    1432-0746

  • e-ISSN

  • Volume of the periodical

    622

  • Issue of the periodical within the volume

    January

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    5

  • Pages from-to

    L8

  • UT code for WoS article

    000457210000001

  • EID of the result in the Scopus database

    2-s2.0-85060970350