PoS - Proceedings of Science
Volume 371 - 7th Annual Conference on High Energy Astrophysics in Southern Africa (HEASA2019) - Modelling II (Chair: Markus Böttcher)
Modelling of synchrotron emission from galaxies and extragalactic radio background
N. Motha* and S. Razzaque
Full text: pdf
Pre-published on: December 15, 2020
Published on: April 02, 2021
Normal galaxies and radio galaxies are associated with star-formation and active galactic nuclei (AGN), respectively. These galaxies are considered to be the primary source of extra-galactic radio emissions permeating throughout the universe. The dominant mechanism responsible for this radio emission is synchrotron radiation due to relativistic electrons interacting with the galactic magnetic field. In this study we calculate the radio spectra from these galaxies. We use observations from the source count population data, which influence the selection of the appropriate radio luminosity function. Finally, we calculate intensity of diffuse extra-galactic radio background using the lambda-CDM cosmology.
DOI: https://doi.org/10.22323/1.371.0014
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