Number of the records: 1  

Radio properties of green pea galaxies

  1. 1.
    0587834 - ASÚ 2025 RIV FR eng J - Journal Article
    Borkar, Abhijeet - Grossová, Romana - Svoboda, Jiří - Moravec, E. - Kouroumpatzakis, Konstantinos - Boorman, P. G. - Adamcová, Barbora - Mingo, B. - Ehle, M.
    Radio properties of green pea galaxies.
    Astronomy & Astrophysics. Roč. 687, July (2024), č. článku A137. ISSN 0004-6361. E-ISSN 1432-0746
    R&D Projects: GA ČR(CZ) GA22-22643S
    Institutional support: RVO:67985815
    Keywords : galaxies: dwarf * galaxies: starburst * galaxies: star formation * radio continuum: galaxies
    OECD category: Astronomy (including astrophysics,space science)
    Impact factor: 6.5, year: 2022
    Method of publishing: Open access

    Aims. Green peas (GPs) are young, compact, star-forming dwarf galaxies, and local (z similar to 0.3) analogues of the early galaxies (z >= 6) considered to be mainly responsible for the reionisation of the Universe. Recent X-ray observations of GPs led to the detection of high excess emission, which cannot be accounted for by star formation alone and implies the presence of an active galactic nucleus (AGN). We employ radio observations to study the radio properties of GPs, build their radio spectral energy distributions, and verify the presence of AGNs.
    Permanent Link: https://hdl.handle.net/11104/0354925

     
    FileDownloadSizeCommentaryVersionAccess
    587834.pdf01 MBPublisher’s postprintopen-access
     
Number of the records: 1  

  This site uses cookies to make them easier to browse. Learn more about how we use cookies.