Hadronic processes in the low-luminosity radio galaxy IC310
The active radio galaxy IC310 is one of brightest objects of the Perseus cluster in the radio wavelengths and X-rays. This source has been detected in radio, X rays and rays. Recently, a -ray flux at TeV energies was detected by the MAGIC Telescopes. We introduce a lepto-hadronic model to describe t...
Guardado en:
| Autores principales: | , , , |
|---|---|
| Formato: | Objeto de conferencia |
| Lenguaje: | Inglés |
| Publicado: |
2015
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/168104 |
| Aporte de: |
| Sumario: | The active radio galaxy IC310 is one of brightest objects of the Perseus cluster in the radio wavelengths and X-rays. This source has been detected in radio, X rays and rays. Recently, a -ray flux at TeV energies was detected by the MAGIC Telescopes. We introduce a lepto-hadronic model to describe the spectral energy distribution (SED), radio to GeV photons as synchrotron self-Compton (SSC) emission and TeV photons as the result of the decay of neutral pions resulting from p interactions. For the p interactions, we assume that the seed photons are those around the second SSC peak. We show that this hadronic model describes successfully the TeV -ray photons at low state of this radio galaxy. Additionally, we compute the number of neutrinos expected to be detected in the IceCube neutrino telescope. |
|---|