  In this work, at first we present a model of studying astrophysical flows of
binary systems and microquasars based on the laws of relativistic
magnetohydrodynamics. Then, by solving the time independent transfer equation,
we estimate the primary and secondary particle distributions within the
hadronic astrophysical jets as well as the emissivities of high energy
neutrinos and $\gamma$-rays. One of our main goals is, by taking into
consideration the various energy-losses of particles into the hadronic jets, to
determine through the transport equation the respective particle distributions
focusing on relativistic hadronic jets of binary systems. As a concrete example
we examine the extragalactic binary system LMC X-1 located in the Large
Magellanic Cloud, a satellite galaxy of our Milky Way Galaxy.
