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Radio properties of green pea galaxies
- 1.0587834 - ASÚ 2025 RIV FR eng J - Článek v odborném periodiku
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
Grant CEP: GA ČR(CZ) GA22-22643S
Institucionální podpora: RVO:67985815
Klíčová slova: galaxies: dwarf * galaxies: starburst * galaxies: star formation * radio continuum: galaxies
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 6.5, rok: 2022
Způsob publikování: 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.
Trvalý link: https://hdl.handle.net/11104/0354925
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