activity
19982015
most citedTwo and Three Dimensional Numerical Simulations of Accretion Discs in a Close Binary System

70 citations · 120 across the 16 of their papers we have counts for

collaborators

16 papers

physics.pop-ph2015★ 1 cited

Confusion around the tidal force and the centrifugal force

Takuya Matsuda, Hiromu Isaka, Henri M. J. Boffin

We discuss the tidal force, whose notion is sometimes misunderstood in the public domain literature. We discuss the tidal force exerted by a secondary point mass on an extended pri…

astro-ph2005

Comments on "Angular Momentum Transport in Quasi-Keplerian Accretion Disks"

Eiji Hayashi, Hiromu Isaka, Takuya Matsuda

Subramanian, Pujari and Becker (2004) claim that the correct expression for the angular momentum transport in an accretion disc, which is proportional to dOmega/dR, can be derived…

astro-ph2004★ 2 cited

On Kinetic Theory Viscosity in a Rotating Gas

Takuya Matsuda, Eiji Hayashi

Clarke and Pringle (2004) derived a proper viscosity formula in a rotating gas by applying mean free path theory. We study their argument in detail and show that their result can b…

astro-ph2004★ 1 cited

Numerical Simulation of the Surface Flow on the Companion Star in a Close Binary System II. Construction of Doppler maps and application to Galactic supersoft X-ray sources

Kazutaka Oka, Takuya Matsuda, Izumi Hachisu +1

We perform three-dimensional numerical simulations of surface flows on the companion star in a semi-detached binary system and construct the corresponding Doppler maps. The mass ra…

astro-ph2004

Gas flow in close binary star systems

K. Oka, T. Matsuda, I. Hachisu +1

We first present a summary of our numerical work on accretion discs in close binary systems. Our recent studies on numerical simulations of the surface flow on the mass-losing star…

astro-ph2002★ 14 cited

Numerical simulation of the surface flow of a companion star in a close binary system

Kazutaka Oka, Takizo Nagae, Takuya Matsuda +2

We simulate numerically the surface flow of a gas-supplying companion star in a semi-detached binary system. Calculations are carried out for a region including only the mass-losin…