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20032008
most citedThree-Dimensional Simulations of Standing Accretion Shock Instability in Core-Collapse Supernovae

140 citations · 234 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph2008★ 80 cited

Effects of Rotation on Standing Accretion Shock Instability in Nonlinear Phase for Core-Collapse Supernovae

Wakana Iwakami, Kei Kotake, Naofumi Ohnishi +2

We studied the effects of rotation on standing accretion shock instability (SASI) by performing three-dimensional hydrodynamics simulations. Taking into account a realistic equatio…

astro-ph2008

The Impact of a Supernova Explosion in a Very Massive Binary

Jun'ichi Sato, Masayuki Umemura, Keisuke Sawada

We consider the effect of a supernova (SN) explosion in a very massive binary that is expected to form in a portion of Population III stars with the mass higher than 100.…

astro-ph2007★ 140 cited

Three-Dimensional Simulations of Standing Accretion Shock Instability in Core-Collapse Supernovae

Wakana Iwakami, Kei Kotake, Naofumi Ohnishi +2

We have studied non-axisymmetric standing accretion shock instability, or SASI, by 3D hydrodynamical simulations. This is an extention of our previous study on axisymmetric SASI. W…

astro-ph2004★ 6 cited

Gas stripping by radiation drag from an interstellar cloud

Jun'ichi Sato, Masayuki Umemura, Keisuke Sawada +1

We perform two-dimensional hydrodynamic simulation on the gas stripping by radiation drag from an interstellar cloud moving in uniform radiation fields. To properly include relativ…

astro-ph2003★ 8 cited

Two-dimensional hydrodynamic simulation of an accretion flow with radiative cooling in a close binary system

Jun'ichi Sato, Keisuke Sawada, Naofumi Ohnishi

Two-dimensional numerical simulations of an accretion flow in a close binary system are performed by solving the Euler equations with radiative transfer. In the present study, the…