Radio Galaxies at TeV Energies

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...

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Detalles Bibliográficos
Otros Autores:	Glawion, Dorit (auth)
Formato:	Libro electrónico
Idioma:	Inglés
Publicado:	MDPI - Multidisciplinary Digital Publishing Institute 2020
Materias:	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
Ver en Biblioteca Universitat Ramon Llull:	https://discovery.url.edu/permalink/34CSUC_URL/1im36ta/alma991009427457606719