Observations of highly inclined disks with ALMA. Results from 12 CO gas and continuum observations

We aim to study the radial and vertical extents of 12 CO gas, millimeter (mm) dust thermal emission and optical/near-infrared scattered light by dust in highly inclined protoplanetary disks. These parameters are indicators of radial drift and vertical settling, and essential to setting better constraints on planet formation. Additionally, we aim to provide estimates of the dynamical stellar masses, including cases where no such prior measurements exist. We analyzed a sample of 14 highly inclined