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

Figure 1

Cooling rates for protons in the jets of M33 X-7 (a) and SS 433 (b) at the base of the jets . The plots of cooling rates show the synchrotron emission (solid lines), the adiabatic cooling (dotted lines), and the inelastic p-p collision rate (dashed lines).

(a)

(b)