Microquasar hadronic jets at very high-energy gamma-rays

Simple item page
dc.creatorBosch-Ramon, V.
dc.creatorAharonian, F. A.
dc.creatorParedes, J. M.
dc.date2006-05-18
dc.date.accessioned2026-07-07T07:08:29Z
dc.date.available2026-07-07T07:08:29Z
dc.descriptionMicroquasars (MQs) present emission over the whole spectrum, from radio wavelengths to gamma-rays. The microquasar spectral energy distribution is very complex, being a signature of the different physical processes that generate the radiation emitted by these objects. In this work, we estimate the amount of broad-band emission produced by relativistic protons, released from the jet of a MQ, interacting with high density regions of the ISM. We show that a two components source, the microquasar itself and the region of interaction between the jets and the ISM, could be unveiled by the new instruments at high-energy and very high-energy gamma-rays.
dc.description4 pages, 2 figures, 1 Table. Proceedings of the Cherenkov 2005 Conference, 27-29 April 2005 - Ecole Polytechnique, Palaiseau, France; edited by B. Degrange, G. Fontaine
dc.identifierhttps://arxiv.org/abs/astro-ph/0605459
dc.identifierhttp://arxiv.org/abs/astro-ph/0605459
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/110726
dc.subjectAstrophysics
dc.titleMicroquasar hadronic jets at very high-energy gamma-rays
dc.typetext

Files

Collections

arXiv