Abstract
With increasingly sharp sub-millimeter direct imaging of transitional disks captured by ALMA, our understanding of the conditions necessary for debris disks to form planetary systems has drastically improved in recent years. Evidence for particle traps in transitional disks suggests that planet formation could possibly take place within density perturbed regions. For this reason we run a grid of models of planet formation in density perturbed transitional disks, and analyze the impact on giant planet formation.
