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A Radio counterpart to a Jupiter-mass binary object in Orion

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A90106%2F24%3A00617494" target="_blank" >RIV/67985815:90106/24:00617494 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.3847/2041-8213/ad18ac" target="_blank" >https://doi.org/10.3847/2041-8213/ad18ac</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.3847/2041-8213/ad18ac" target="_blank" >10.3847/2041-8213/ad18ac</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    A Radio counterpart to a Jupiter-mass binary object in Orion

  • Original language description

    Using James Webb Space Telescope near-infrared data of the inner Orion Nebula, Pearson & McCaughrean detected 40 Jupiter-mass binary objects (JuMBOs). These systems are not associated with stars and their components have masses of giant Jupiter-like planets and separations in the plane of the sky of order similar to 100 au. The existence of these wide free-floating planetary-mass binaries was unexpected in our current theories of star and planet formation. Here we report the radio continuum (6.1 and 10.0 GHz) Karl G. Jansky Very Large Array detection of a counterpart to JuMBO 24. The radio emission appears to be steady at a level of similar to 50 mu Jy over timescales of days and years. We set an upper limit of similar or equal to 15 km s-1 to the velocity of the radio source in the plane of the sky. As in the near-infrared, the radio emission seems to be coming from both components of the binary.

  • 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

  • Continuities

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

    Astrophysical Journal Letters

  • ISSN

    2041-8205

  • e-ISSN

    2041-8213

  • Volume of the periodical

    960

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    5

  • Pages from-to

    L14

  • UT code for WoS article

    001138148700001

  • EID of the result in the Scopus database

    2-s2.0-85182368871