The Ophiuchus DIsc Survey Employing ALMA (ODISEA). Substructures as a function of SED Class and disc mass in 100 systems
The Ophiuchus DIsc Survey (ODISEA) is a study of 100 protoplanetary disks using ALMA. Researchers found that more massive disks are more likely to show evolved substructures, such as gap-ring pairs. This work provides a baseline for characterizing disk evolution and predicting where giant planet cores should form.