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Gamma-ray emission in radio galaxies, from MeV to TeV

Published online by Cambridge University Press:  07 April 2020

Eleonora Torresi
Eleonora Torresi*
Affiliation:
Dipartimento di Astronomia, Università di Bologna, via Gobetti, 93/2, I-40129, Bologna, Italy INAF-OAS Bologna, Area della Ricerca CNR, via Gobetti, 101, I-40129, Bologna, Italy email: [email protected]
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Abstract

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Thanks to the Fermi λ-ray satellite and the current Imaging Atmospheric Cherenkov Telescopes, radio galaxies have arisen as a new class of high- and very-high energy emitters. The favourable orientation of their jets makes radio galaxies extremely relevant in addressing important issues such as: (i) revealing the jet structure complexity; (ii) localising the emitting region(s) of high- and very-high energy radiation; (iii) understanding the physical processes producing these photons. In this review the main results on the λ-ray emission studies of radio galaxies from the MeV to TeV regimes will be presented, and the impact of future Cherenkov Telescope Array observations will be discussed.

Keywords

radiation mechanisms: nonthermalgalaxies: activegalaxies: jetsgalaxies: nuclei
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S342: Perseus in Sicily: From Black Hole to Cluster Outskirts , May 2018 , pp. 158 - 166
Copyright
© International Astronomical Union 2020

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