Radio properties of green pea galaxies

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00587834" target="_blank" >RIV/67985815:_____/24:00587834 - isvavai.cz</a>
Alternative codes found
RIV/00216224:14310/24:00136708
Result on the web
<a href="https://hdl.handle.net/11104/0354925" target="_blank" >https://hdl.handle.net/11104/0354925</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202348819" target="_blank" >10.1051/0004-6361/202348819</a>

Result language
angličtina
Original language name
Radio properties of green pea galaxies
Original language description
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.
Czech name
—
Czech description
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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)

Project
<a href="/en/project/GA22-22643S" target="_blank" >GA22-22643S: Galactic gastronomy: Green Peas and Blueberries</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2024
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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