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A case for a binary black hole system revealed via quasi-periodic outflows

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00586709" target="_blank" >RIV/67985815:_____/24:00586709 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216224:14310/24:00135880 RIV/00216208:11320/24:10492425

  • Result on the web

    <a href="https://hdl.handle.net/11104/0354150" target="_blank" >https://hdl.handle.net/11104/0354150</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1126/sciadv.adj8898" target="_blank" >10.1126/sciadv.adj8898</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    A case for a binary black hole system revealed via quasi-periodic outflows

  • Original language description

    Binaries containing a compact object orbiting a supermassive black hole are thought to be precursors of gravitational wave events, but their identification has been extremely challenging. Here, we report quasi-periodic variability in x-ray absorption, which we interpret as quasi-periodic outflows (QPOuts) from a previously low-luminosity active galactic nucleus after an outburst, likely caused by a stellar tidal disruption. We rule out several models based on observed properties and instead show using general relativistic magnetohydrodynamic simulations that QPOuts, separated by roughly 8.3 days, can be explained with an intermediate-mass black hole secondary on a mildly eccentric orbit at a mean distance of about 100 gravitational radii from the primary. Our work suggests that QPOuts could be a new way to identify intermediate/extreme-mass ratio binary candidates.

  • 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

    <a href="/en/project/GM24-10599M" target="_blank" >GM24-10599M: Stars in galactic nuclei: interrelation with massive black holes</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Science Advances

  • ISSN

    2375-2548

  • e-ISSN

    2375-2548

  • Volume of the periodical

    10

  • Issue of the periodical within the volume

    13

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    22

  • Pages from-to

    eadj8898

  • UT code for WoS article

    001193309500002

  • EID of the result in the Scopus database

    2-s2.0-85189382802