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Leptonic emission from microquasar jets: from radio to very high-energy gamma-rays

Published online by Cambridge University Press:  12 May 2006

Valentí Bosch-Ramon ,
Josep M. Paredes  and
Gustavo E. Romero
Valentí Bosch-Ramon
Affiliation:
Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Av. Diagonal 647, E-08028 Barcelona, Catalonia (Spain) email: vbosch@am.ub.es
Josep M. Paredes
Affiliation:
Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Av. Diagonal 647, E-08028 Barcelona, Catalonia (Spain) email: vbosch@am.ub.es
Gustavo E. Romero
Affiliation:
Instituto Argentino de Radioastronomía, C.C.5, (1894) Villa Elisa, Buenos Aires (Argentina) Facultad de Ciencias Astronómicas y Geofísicas, UNLP, Paseo del Bosque, 1900 La Plata (Argentina)
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Abstract

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Microquasars are sources of very high-energy gamma-rays and, very probably, high-energy gamma-ray emitters. We propose a model for a jet that can allow to give accurate observational predictions for jet emission at different energies and provide with physical information of the object using multiwavelength data.

Keywords

X-rays: binariesgamma rays: theorygamma rays: observations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S230: Populations of High Energy Sources in Galaxies , August 2005 , pp. 91 - 92
Copyright
2006 International Astronomical Union