Extending dynamical mass measurements: probing GI as a possible origin of mm-dust spirals

Constraining the total mass of protoplanetary disks is crucial to determine the availability of material for planet formation.

Constraining the total mass of protoplanetary disks is crucial to determine the availability of material for planet formation. Yet, providing accurate and precise measurements of the disk mass is challenging. Investigating the gas dynamics is a powerful, tracer-independent…