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Global Structure of Three Distinct Accretion Flows and Outflows around Black Holes from Two-dimensional Radiation-magnetohydrodynamic Simulations

The Astrophysical journal, 2011-07, Vol.736 (1), p.2-jQuery1323905823926='48'

2011

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General Relativistic Radiation Magnetohydrodynamics Simulations of Black Hole Accretion Disks: Comparison of Methods Based on Variable Eddington Tensor and Based on M1 Closure

The Astrophysical journal, 2022-04, Vol.929 (1), p.93

2022

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General Relativistic Radiation Magnetohydrodynamics Simulations of Precessing Tilted Super-Eddington Disks

The Astrophysical journal, 2024-09, Vol.973 (1), p.45

2024

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The origins and impact of outflow from super-Eddington flow

Publications of the Astronomical Society of Japan, 2021-04, Vol.73 (2), p.450-466

2021

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Super-critical column accretion on to strongly magnetized neutron stars in ULX pulsars

Publications of the Astronomical Society of Japan, 2020-02, Vol.72 (1)

2020

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Clumpy Outflows from Supercritical Accretion Flow

Publications of the Astronomical Society of Japan, 2013-08, Vol.65 (4)

2013

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Radio Images inside Highly Magnetized Jet Funnels Based on Semianalytic GRMHD Models

The Astrophysical journal, 2024-07, Vol.969 (1), p.22

2024

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FORMATION OF OVERHEATED REGIONS AND TRUNCATED DISKS AROUND BLACK HOLES: THREE-DIMENSIONAL GENERAL RELATIVISTIC RADIATION-MAGNETOHYDRODYNAMICS SIMULATIONS

The Astrophysical journal, 2016-07, Vol.826 (1), p.23-23

2016

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General Relativistic Radiation MHD Simulations of Supercritical Accretion onto a Magnetized Neutron Star: Modeling of Ultraluminous X-Ray Pulsars

Astrophysical journal. Letters, 2017-08, Vol.845 (1), p.L9

2017

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The thermal-radiative wind in low-mass X-ray binary H1743−322 – II. Iron line predictions from Monte Carlo radiation transfer

Monthly notices of the Royal Astronomical Society, 2020-05, Vol.494 (3), p.3413-3421

2020

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A radiation-hydrodynamics model of accretion columns for ultra-luminous X-ray pulsars

Publications of the Astronomical Society of Japan, 2016-10, Vol.68 (5)

2016

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RAIKOU (来光): A General Relativistic, Multiwavelength Radiative Transfer Code

The Astrophysical journal, 2023-06, Vol.949 (2), p.101

2023

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

Publications of the Astronomical Society of Japan, 2022-12, Vol.74 (6), p.1378-1395

2022

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A Numerical Scheme for General Relativistic Radiation Magnetohydrodynamics Based on Solving a Grid-based Boltzmann Equation

The Astrophysical journal, 2020-10, Vol.901 (2), p.96

2020

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The thermal-radiative wind in the neutron star low-mass X-ray binary GX 13 + 1

Monthly notices of the Royal Astronomical Society, 2020-10, Vol.497 (4), p.4970-4980

2020

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Radiation drag effects in black hole outflows from super-critical accretion disks via special relativistic radiation magnetohydrodynamics simulations

Publications of the Astronomical Society of Japan, 2015-08, Vol.67 (4)

2015

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Polarization images of accretion flow around supermassive black holes: Imprints of toroidal field structure

Publications of the Astronomical Society of Japan, 2021-08, Vol.73 (4), p.912-928

2021

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Component of Energy Flow from Supercritical Accretion Disks Around Rotating Stellar Mass Black Holes

The Astrophysical journal, 2022-08, Vol.935 (1), p.26

2022

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Theoretical modeling of Comptonized X-ray spectra of super-Eddington accretion flow: Origin of hard excess in ultraluminous X-ray sources

Publications of the Astronomical Society of Japan, 2017-12, Vol.69 (6)

2017

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Modeling of Thermal Emission from ULX Pulsar Swift J0243.6+6124 with General Relativistic Radiation MHD Simulations

The Astrophysical journal, 2023-07, Vol.952 (1), p.62

2023

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A NUMERICAL SCHEME FOR SPECIAL RELATIVISTIC RADIATION MAGNETOHYDRODYNAMICS BASED ON SOLVING THE TIME-DEPENDENT RADIATIVE TRANSFER EQUATION

The Astrophysical journal, 2016-02, Vol.818 (2), p.162

2016

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Structure of the super-Eddington outflow and its impact on the cosmological scale

Publications of the Astronomical Society of Japan, 2022-04, Vol.74 (2), p.384-397

2022

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Variability of Comptonized X-ray spectra of a super-Eddington accretor: Approach using Boltzmann radiation transport

Publications of the Astronomical Society of Japan, 2021-06, Vol.73 (3), p.701-715

2021

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Radiation MHD Simulations of Soft X-Ray Emitting Regions in Changing Look AGN

The Astrophysical journal, 2024-06, Vol.968 (2), p.121

2024

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Pulsed fraction of super-critical column accretion flows on to neutron stars: Modeling of ultraluminous X-ray pulsars

Publications of the Astronomical Society of Japan, 2020-04, Vol.72 (2)

2020

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Global Structure of Three Distinct Accretion Flows and Outflows around Black Holes from Two-dimensional Radiation-magnetohydrodynamic Simulations

General Relativistic Radiation Magnetohydrodynamics Simulations of Black Hole Accretion Disks: Comparison of Methods Based on Variable Eddington Tensor and Based on M1 Closure

General Relativistic Radiation Magnetohydrodynamics Simulations of Precessing Tilted Super-Eddington Disks

The origins and impact of outflow from super-Eddington flow

Super-critical column accretion on to strongly magnetized neutron stars in ULX pulsars

Clumpy Outflows from Supercritical Accretion Flow

Radio Images inside Highly Magnetized Jet Funnels Based on Semianalytic GRMHD Models

FORMATION OF OVERHEATED REGIONS AND TRUNCATED DISKS AROUND BLACK HOLES: THREE-DIMENSIONAL GENERAL RELATIVISTIC RADIATION-MAGNETOHYDRODYNAMICS SIMULATIONS

General Relativistic Radiation MHD Simulations of Supercritical Accretion onto a Magnetized Neutron Star: Modeling of Ultraluminous X-Ray Pulsars

The thermal-radiative wind in low-mass X-ray binary H1743−322 – II. Iron line predictions from Monte Carlo radiation transfer

A radiation-hydrodynamics model of accretion columns for ultra-luminous X-ray pulsars

RAIKOU (来光): A General Relativistic, Multiwavelength Radiative Transfer Code

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

A Numerical Scheme for General Relativistic Radiation Magnetohydrodynamics Based on Solving a Grid-based Boltzmann Equation

The thermal-radiative wind in the neutron star low-mass X-ray binary GX 13 + 1

Radiation drag effects in black hole outflows from super-critical accretion disks via special relativistic radiation magnetohydrodynamics simulations

Polarization images of accretion flow around supermassive black holes: Imprints of toroidal field structure

Component of Energy Flow from Supercritical Accretion Disks Around Rotating Stellar Mass Black Holes

Theoretical modeling of Comptonized X-ray spectra of super-Eddington accretion flow: Origin of hard excess in ultraluminous X-ray sources

Modeling of Thermal Emission from ULX Pulsar Swift J0243.6+6124 with General Relativistic Radiation MHD Simulations

A NUMERICAL SCHEME FOR SPECIAL RELATIVISTIC RADIATION MAGNETOHYDRODYNAMICS BASED ON SOLVING THE TIME-DEPENDENT RADIATIVE TRANSFER EQUATION

Structure of the super-Eddington outflow and its impact on the cosmological scale

Variability of Comptonized X-ray spectra of a super-Eddington accretor: Approach using Boltzmann radiation transport

Radiation MHD Simulations of Soft X-Ray Emitting Regions in Changing Look AGN

Pulsed fraction of super-critical column accretion flows on to neutron stars: Modeling of ultraluminous X-ray pulsars

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