64 citations · 80 across the 4 of their papers we have counts for
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3D Gasdynamic Modelling of the Changes in the Flow Structure During Transition From Quiescent to Active State in Symbiotic Stars
M. Mitsumoto, B. Jahanara, T. Matsuda +6
The results of 3D modelling of the flow structure in the classical symbiotic system Z~Andromedae are presented. Outbursts in systems of this type occur when the accretion rate exce…
Wind accretion in binary stars - I. Mass accretion ratio
T. Nagae, K. Oka, T. Matsuda +3
Three-dimensional hydrodynamic calculations are performed in order to investigate mass transfer in a close binary system, in which one component undergoes mass loss through a wind.…
Direct Monte Carlo simulations of accretion discs
Takuya Matsuda, Hiromi Mizutani, Henri M. J. Boffin
We apply the Direct Simulation Monte Carlo (DSMC) method, developed originally to calculate rarefied gas dynamical problems, to study the gas flow in an accretion disc in a close b…
Spiral Shocks in 3D Accretion Discs
Hiroshi Yukawa, Henri M. J. Boffin, Takuya Matsuda
We have performed three-dimensional numerical simulations of accretion discs in a close binary system using the Smoothed Particle Hydrodynamics method. Our result show that, contra…