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Microquasars as Sources of High Energy Phenomena

Published online by Cambridge University Press:  26 May 2016

I. F. Mirabel
I. F. Mirabel*
Affiliation:
Centre d'Etudes de Saclay/CEA/DSM/DAPNIA/SAP 91911 Gif/Yvette, France & Intituto de Astronomía y Física del Espacio/CONICET, Argentina

Abstract

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Relativistic 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.

Type
Part 6 X-Ray Binaries
Information
Symposium - International Astronomical Union , Volume 214: High Energy Processes and Phenomena in Astrophysics , 2003 , pp. 201 - 210
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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