- Conference date: 26-30 Jun 2000
- Location: Heidelberg (Germany)
Based on the results of detailed modelling of the powerful radio flare of the microquasar GRS in March/April 1994, here we discuss γ-ray fluxes which can be expected from this class of objects. We discuss also perspectives and possible strategy for detection of microquasars in high and very high energy gamma-rays.
- Gamma rays
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