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Radiation processes around accreting black holes
R. Belmont, J. Malzac, A. Marcowith
Accreting sources such as AGN, X-ray binaries or gamma-ray bursts are known to be strong, high energy emitters. The hard emission is though to originate from plasmas of thermal and…
Simulating acceleration and radiation processes in X-ray binaries
R. Belmont, J. Malzac, A. Marcowith
The high energy emission of microquasars is thought to originate from high energy particles. Depending on the spectral state, the distribution of these particles can be thermal wit…
A new code for radiation processes in high energy plasmas
R. Belmont, J. Malzac, A. Marcowith
Extreme objects such as X-ray binaries, AGN, or -ray bursters harbor high energy plasmas whose properties are not well understood yet. Not only are they responsible of the hard…
Accretion discs, coronae and jets in black hole binaries: prospects for Simbol-X
Julien Malzac
The phenomenology of accretion disc, coronnae and jets in X-ray binaries is rather well established. However the structure of the accretion flow in the various spectral states is s…
Jet disc coupling in black hole binaries
Julien Malzac
In the last decade multi-wavelength observations have demonstrated the importance of jets in the energy output of accreting black hole binaries. The observed correlations between t…