205 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Novosibirsk State UniversityRU17 papers
- Siberian Branch of the Russian Academy of SciencesRU11 papers
- Russian Academy of SciencesRU9 papers
- Institute of Semiconductor PhysicsRU6 papers
- Nikolaev Institute of Inorganic ChemistryRU5 papers
- CJSC Ekran FEP (Russia)RU3 papers
- Hiroshima UniversityJP3 papers
- Institute of Computational Mathematics and Mathematical GeophysicsRU3 papers
- Institute of Strength Physics and Materials ScienceRU3 papers
- Lomonosov Moscow State UniversityRU3 papers
- Novosibirsk State Technical UniversityRU3 papers
- Southern Federal UniversityRU3 papers
6 papers · 1 filter
Development and application of fast methods for computing momentum transfer between gas and dust in supercomputer simulation of planet formation
Olga P. Stoyanovskaya, Vitaly V. Akimkin, Eduard I. Vorobyov +4
Circumstellar discs, from which planetary systems are formed, consist of gas, dust and solids. Simulations of self-consistent dynamics of gas, dust and solids in circumstellar disc…
Two-Fluid Dusty Gas in Smoothed Particle Hydrodynamics: Fast and Implicit Algorithm for Stiff Linear Drag
Olga P. Stoyanovskaya, Tatiana A. Glushko, Nikolay V. Snytnikov +1
Simulation of the dynamics of dust-gas circumstellar discs is crucial in understanding the mechanisms of planet formation. The dynamics of small grains in the disc is stiffly coupl…
Modeling Circumstellar Disc Fragmentation and Episodic Protostellar Accretion with Smoothed Particle Hydrodynamics in Cell
Olga P. Stoyanovskaya, Nikolay V. Snytnikov, Valeriy N. Snytnikov
We discuss the ability of the smoothed particle hydrodynamics (SPH) method combined with a grid-based solver for the Poisson equation to model mass accretion onto protostars in gra…
Analysis of Numerical Algorithms for Computing Rapid Momentum Transfers between the Gas and Dust in Simulations of Circumstellar Disks
O. P. Stoyanovskaya, E. I. Vorobyov, V. N. Snytnikov
Approaches used in modern numerical simulations of the dynamics of dust and gas in circumstellar disks are tested. The gas and dust are treated like interpenetrating continuous med…
The early evolution of viscous and self-gravitating circumstellar disks with a dust component
Eduard Vorobyov, Vitaly Akimkin, Olga Stoyanovskaya +2
The long-term evolution of a circumstellar disk starting from its formation and ending in the T Tauri phase was simulated numerically with the purpose of studying the evolution of…
Clump formation due to the gravitational instability of a multiphase medium in a massive protoplanetary disc
Valeriy N. Snytnikov, Olga P. Stoyanovskaya
Planetary systems form in gas-dust protoplanetary discs via the growth of solid bodies. In this paper, we show that the most intriguing stage of such growth --- namely, the transfo…