Molecular emission from a protostellar jet-disk wind interaction

Protostellar jets are common signatures shown by very young protostars. This high-velocity jet and the cavity comprise a molecular outflow that, additionally, could interact with the wind generated by the circumstellar disk wind that surrounds the protostar. We are interested in studying the interaction between the jet and a disk wind, considering their molecular evolution. We used WALKIMYA-2D, axisymmetric chemo- hydrodynamical code, to simulate the interaction between the jet, disk wind, and the environment