Microquasars as sources of high energy phenomena

Simple item page
dc.creatorMirabel, I. F.
dc.date2002-11-05
dc.date.accessioned2026-07-07T02:06:01Z
dc.date.available2026-07-07T02:06:01Z
dc.descriptionRelativistic outflows are a common phenomenon in accreting black holes. Despite the enormous differences in scale, accreting stellar-mass black holes (X-ray binaries, collapsars) and super-massive black holes produce jets with analogous physical properties. Here I review microquasars as sources of relativistic jets, gamma-rays, cosmic rays, and high energy neutrinos.
dc.description10 pages, 2 figures. Invited review at the IAU Symposium No.214: High Energy Processes and Phenomena in Astrophysics
dc.identifierhttps://arxiv.org/abs/astro-ph/0211085
dc.identifierhttp://arxiv.org/abs/astro-ph/0211085
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5285
dc.subjectAstrophysics
dc.titleMicroquasars as sources of high energy phenomena
dc.typetext

Files

Collections

arXiv