Modeling Particle Transport in Astrophysical Outflows and Simulations of Associated Emissions from Hadronic Microquasar Jets

Figure 5

Pion (a) and muon (b) distributions for M33 X-7. In both cases of particles-, we compare the distribution which considers the important energy losses and with that which neglects energy losses for . Both types of particle distributions refer to the base of the jet, i.e., at .

(a)

(b)