TY  - JOUR
AU  - O. P. Stoyanovskaya
TI  - Numerical simulation of gravitational instability development and clump formation in massive circumstellar disks using integral characteristics for the interpretation of results
JO  - Numerical methods and programming
PY  - 2016
SP  - 339
EP  - 352
VL  - 17
IS  - 3
PB  - mathdoc
UR  - http://geodesic.mathdoc.fr/item/VMP_2016_17_3_a14/
LA  - ru
ID  - VMP_2016_17_3_a14
ER  -