Stoyanovskaya O. Numerical simulation of gravitational instability development and clump formation in massive circumstellar disks using integral characteristics for the interpretation of results. Num. Meth. Prog. [Internet]. 2016 Aug. 23 [cited 2024 Apr. 25];17(49):339-52. Available from: https://en.num-meth.ru/index.php/journal/article/view/895