Abstract
The jet in a microquasar stellar system is simulated with a relativistic hydrocode (PLUTO) and then it is imaged, in the γ-rays wave band, with a line-of-sight method, including both emission and self-absorption. A synthetic image is produced which allows to better estimate the system's physical properties. The calculation procedure in our method has been simplified by exploiting the ability to de-couple the hydrodynamical from the radiative quantities in the computations.
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