To the question of astrophysical studies of protoplanetary disks of stars
Abstract:
A brief analytical review of selected works on astrophysical observations of protoplanetary disks of stars is presented. It is shown that the data of astrophysical studies generally confirm the validity of the model of protoplanetary rings - the model of formation of planetary systems of stars, which is based on the origin and development of large-scale gravitational instability (protoplanetary rings) in the protoplanetary disks of stars.
