45 citations · 70 across the 5 of their papers we have counts for
5 papers
Impact of Ly radiation force on super-Eddington accretion onto a massive black hole
Takuya Mushano, Takumi Ogawa, Ken Ohsuga +2
The viability of super-Eddington accretion remains a topic of intense debate, crucial for understanding the formation of supermassive black holes in the early universe. However, th…
3D Photon Conserving Code for Time-dependent General Relativistic Radiative Transfer : CARTOON
Mikiya M. Takahashi, Ken Ohsuga, Rohta Takahashi +3
We develop the 3-dimensional general relativistic radiative transfer code: CARTOON (Calculation code of Authentic Radiative Transfer based On phOton Number conservation in curved s…
Matter density distribution of general relativistic highly magnetized jets driven by black holes
Taiki Ogihara, Takumi Ogawa, Kenji Toma
High-resolution very long baseline interferometry (VLBI) radio observations have resolved the detailed emission structures of active galactic nucleus jets. General relativistic mag…
Monte Carlo studies of the spin-chirality decoupling in the three-dimensional Heisenberg spin glass
Takumi Ogawa, Kazuki Uematsu, Hikaru Kawamura
An extensive equilibrium Monte Carlo simulation is performed on the 3D isotropic Heisenberg SG model with the random nearest-neighbor Gaussian coupling, with particular interest in…
A radiation-hydrodynamic model of accretion columns for ultra-luminous X-ray pulsars
Tomohisa Kawashima, Shin Mineshige, Ken Ohsuga +1
Prompted by the recent discovery of pulsed emission from an ultra-luminous X-ray source, M82 X-2 ("ULX-pulsar"), we perform a two-dimensional radiation-hydrodynamic simulation of a…