Analysis of Methods for Computing the Trajectories of Dust Particles in a Gas–Dust Circumstellar Disk › Research Explorer

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Analysis of Methods for Computing the Trajectories of Dust Particles in a Gas–Dust Circumstellar Disk

Research output: Contribution to journal › Article › peer-review

Energy-Saving Catalytic Processes Laboratory

DOI

https://doi.org/10.1134/S1063772917120071
Final published version

O. P. Stoyanovskaya
V. N. Snytnikov
E. I. Vorobyov

Original language	English
Pages (from-to)	1044-1060
Number of pages	17
Journal	Astronomy Reports
Volume	61
Issue number	12
DOIs	https://doi.org/10.1134/S1063772917120071
Publication status	Published - 1 Dec 2017

Research areas

PROTOPLANETARY DISKS, GRAVITATIONAL-INSTABILITY, SEMIIMPLICIT APPROACH, SOLID PARTICLES, SOLAR NEBULA, 2-FLUID DUST, MIXTURES, HYDRODYNAMICS, SIMULATION, GROWTH

OECD FOS+WOS

ID: 9640529