The Burst Mode of Accretion of Massive Circumstellar Disc: Simulations with Smoothed Particle Hydrodynamics and Grid-Based Gravitational Solver | Sciact - CRIS-system of Boreskov Institute of Catalysis

The Burst Mode of Accretion of Massive Circumstellar Disc: Simulations with Smoothed Particle Hydrodynamics and Grid-Based Gravitational Solver Conference Abstracts

Conference

The Conference "Disc Dynamics and Planet Formation"
29 Jun - 3 Jul 2015 , Larnaka

Source

Book of abstracts "Disc dynamics and planet formation"
Compilation, 2015.

Output data

Year: 2015, Pages: 200 Pages count : 1

Authors

Stoyanovskaya O.P. ^1,2 , Vorobyov E.I. ⁴ , Snytnikov N.V. ³ , Snytnikov V.N. ^1,2

Affiliations

1	Boreskov Institute of Catalysis SB RAS
2	Novosibirsk National Research University
3	Institute of Computational Mathematics and Mathematical Geophysics SB RAS
4	Universitat Wien

Stoyanovskaya O.P. , Vorobyov E.I. , Snytnikov N.V. , Snytnikov V.N.
The Burst Mode of Accretion of Massive Circumstellar Disc: Simulations with Smoothed Particle Hydrodynamics and Grid-Based Gravitational Solver
In compilation Book of abstracts "Disc dynamics and planet formation". 2015. – C.200.

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