Protostellar jets are present in the later stages of the stellar formation. Non-thermal radio emission has been detected from the jets and hot spots of some massive protostars, indicating the presence of relativistic electrons there. We are intereste
d in exploring if these non-thermal particles can emit also at gamma-rays. In the present contribution we model the non-thermal emission produced in the jets associated with the massive protostar IRAS 18162-2048. We obtain that the gamma-ray emission produced in this source is detectable by the current facilities in the GeV domain.
