Radio Galaxies at TeV Energies

• Váldodahkki: Glawion, Dorit (auth)
• Materiálatiipa: Elektrovnnalaš Girjji oassi
• Giella: eaŋgalasgiella
• Almmustuhtton: MDPI - Multidisciplinary Digital Publishing Institute 2020
• Fáttát: Astronomy, space & time; radiation mechanisms: non-thermal; emission: non-thermal; 3C 84; radio galaxies; TeV ?-rays; X-rays: binaries; general relativity; jets; Centaurus A; light curve; particle acceleration; galaxies: active; discrete correlation function; relativistic processes ISM: jets and outflows; VLBA; origin: jet; stars: black holes; GeV ?-rays; galaxies: jets; magnetohydrodynamics; active galactic nuclei; radio galaxy; origin: black hole; TeV emission; radio interferometry; gamma-rays; gamma-rays: observation; gamma-rays: theory; active galactic nucleus
• Liŋkkat: DOAB: download the publication; DOAB: description of the publication

It is common believe that the centers of all galaxies exhibit supermassive black holes with masses ranging from millions up to billions of the mass of our Sun. By accreting surrounding matter, the luminosity of these galactic nuclei can outshine the emission of their host galaxies. If this is the ca...