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We investigate the production of gamma-rays in the inner regions of SS 433and in its interaction between its jets and the W50 nebula. We estimate the VHEemission that can be generated within the jets at distances above 1e+13 cm fromthe compact object. We also apply a theoretical model of the jet/mediuminteraction to SS 433/W50. We compare the predicted fluxes to observations ofSS 433 at TeV energies, and derive new constraints of the physical propertiesof this system.

Gamma-rays from SS~433 and its interaction with the W50 nebula