| Transition disks, positioned between primordial protoplanetary and debris disks, are pivotal in studying planet formation. In this work we are focusing on the exploration of small-scale substructures within these disks using high-resolution data from ALMA. By examining features such as rings, gaps, and cavities, we can advance our understanding of the disk-planet interactions and other evolutionary features. Our study encompasses a wide range of masses, aiming to uncover how these structures vary with stellar and disk properties. |
