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We present results of hydrodynamic simulations of star formation triggered bycloud-cloud collisions. During the early stages of star formation, low-massobjects form by gravitational instabilities in protostellar discs. A number ofthese low-mass objects are in the sub-stellar mass range, including a fewobjects of planetary mass. The disc instabilities that lead to the formation oflow-mass objects in our simulations are the product of disc-disc interactionsand/or interactions between the discs and their surrounding gas.

SPH simulations of star/planet formation triggered by cloud-cloud collisions