activity
20172024
most citedSystematic two-dimensional radiation hydrodynamic simulations of super-Eddington accretion flow and outflow: Comparison with the slim disk model

45 citations · 116 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2024

Radiation and outflow properties of super-Eddington accretion flows around various mass classes of black holes: Dependence on the accretion rates

Shogo Yoshioka, Shin Mineshige, Ken Ohsuga +2

We perform axisymmetric two-dimensional radiation-hydrodynamic simulations of super-Eddington accretion flow and outflow around black holes to examine the properties of radiation a…

astro-ph.HE2022★ 28 cited

Large-scale outflow structure and radiation properties of super-Eddington flow: Dependence on the accretion rates

Shogo Yoshioka, Shin Mineshige, Ken Ohsuga +2

In order to precisely evaluate the impacts by super-Eddington accretors to their environments, it is essential to assure a large enough simulation box and long computational time t…

astro-ph.GA2022★ 7 cited

Structure of the super-Eddington outflow and itsimpact on the cosmological scale

Ignacio Botella, Shin Mineshige, Takaaki Kitaki +2

It is one of the biggest issues in black hole (BH) astrophysics how to precisely evaluate BH feedback to its environments. Aiming at studying the unique gas dynamics of super-Eddin…

astro-ph.HE2021★ 5 cited

Outflow from super-Eddington flow: where it originates from and how much impact it gives?

Takaaki Kitaki, Shin Mineshige, Ken Ohsuga +1

It is widely believed that super-Eddington accretion flow can produce powerful outflow, but where it originates from and how much mass and energy are carried away to which directio…

astro-ph.HE2018★ 45 cited

Systematic two-dimensional radiation hydrodynamic simulations of super-Eddington accretion flow and outflow: Comparison with the slim disk model

Takaaki Kitaki, Shin Mineshige, Ken Ohsuga +1

To what extent can the one-dimensional slim disk model reproduce the multi-dimensional results of global radiation-hydrodynamic simulations of super-Eddington accretion? With this…

astro-ph.HE2017★ 31 cited

Theoretical modeling of Comptonized X-ray spectra of super-Eddington accretion flow: origin of hard excess in Ultraluminous X-Ray Sources

Takaaki Kitaki, Shin Mineshige, Ken Ohsuga +1

X-ray continuum spectra of super-Eddington accretion flow are studied by means of Monte Carlo radiative transfer simulations based on the radiation hydrodynamic simulation data, in…