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25 Years of Self-Organized Criticality: Solar and Astrophysics.
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- Space Science Reviews, 2016, v. 198, n. 1-4, p. 47, doi. 10.1007/s11214-014-0054-6
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- Article
Outflow Launching Mechanisms.
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- Space Science Reviews, 2014, v. 183, n. 1-4, p. 353, doi. 10.1007/s11214-013-0017-3
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- Article
Study of the Time-Series of Microvariability in Kepler Blazar W2R 1926+42.
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- Galaxies (2075-4434), 2017, v. 5, n. 1, p. 13, doi. 10.3390/galaxies5010013
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- Article
Radiation and outflow properties of super-Eddington accretion flows around various mass classes of black holes: Dependence on the accretion rates.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 5, p. 1015, doi. 10.1093/pasj/psae067
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- Article
Model of a "Warm Corona" as the origin of the soft X-ray excess of active galactic nuclei.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 2, p. 306, doi. 10.1093/pasj/psae012
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- Article
Evolution of accretion disk structure of the black hole X-ray binary MAXI J1820+070 during the rebrightening phase.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 2, p. 251, doi. 10.1093/pasj/psae005
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Large-scale outflow structure and radiation properties of super-Eddington flow: Dependence on the accretion rates.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 6, p. 1378, doi. 10.1093/pasj/psac076
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Multiwavelength observations of the black hole X-ray binary MAXI J1820+070 in the rebrightening phase.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 4, p. 805, doi. 10.1093/pasj/psac038
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Structure of the super-Eddington outflow and its impact on the cosmological scale.
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- Publications of the Astronomical Society of Japan, 2022, v. 74, n. 2, p. 384, doi. 10.1093/pasj/psac001
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- Article
Polarization images of accretion flow around supermassive black holes: Imprints of toroidal field structure.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, n. 4, p. 912, doi. 10.1093/pasj/psab054
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Variability of Comptonized X-ray spectra of a super-Eddington accretor: Approach using Boltzmann radiation transport.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, n. 3, p. 701, doi. 10.1093/pasj/psab031
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What determines the unique spectra of super-Eddington accretors? Origin of optically thick and low-temperature coronae in super-Eddington accretion flows.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, n. 3, p. 630, doi. 10.1093/pasj/psab023
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The origins and impact of outflow from super-Eddington flow.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, n. 2, p. 450, doi. 10.1093/pasj/psab011
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Systematic two-dimensional radiation-hydrodynamic simulations of super-Eddington accretion flow and outflow: Comparison with the slim disk model.
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- Publications of the Astronomical Society of Japan, 2018, v. 70, n. 6, p. N.PAG, doi. 10.1093/pasj/psy110
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- Article
Can the relativistic light-bending model explain X-ray spectral variations of Seyfert galaxies?
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- Publications of the Astronomical Society of Japan, 2018, v. 70, n. 3, p. 42-1, doi. 10.1093/pasj/psy032
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- Article
Three-dimensional structure of clumpy outflow from supercritical accretion flow onto black holes.
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- Publications of the Astronomical Society of Japan, 2018, v. 70, n. 2, p. 1, doi. 10.1093/pasj/psx157
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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.
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- Publications of the Astronomical Society of Japan, 2017, v. 69, n. 6, p. 1, doi. 10.1093/pasj/psx101
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Radiation hydrodynamic simulations of a super-Eddington accretor as a model for ultra-luminous sources.
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- Publications of the Astronomical Society of Japan, 2017, v. 69, n. 2, p. 1, doi. 10.1093/pasj/psx006
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A radiation-hydrodynamics model of accretion columns for ultra-luminous X-ray pulsars.
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- Publications of the Astronomical Society of Japan, 2016, v. 68, n. 5, p. 1, doi. 10.1093/pasj/psw075
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New method for probing Kerr space-time based on imaging observation of in-falling gas blob.
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- Publications of the Astronomical Society of Japan, 2016, v. 68, n. 3, p. 1, doi. 10.1093/pasj/psw019
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New method for black-hole spin measurement based on flux variation from an infalling gas ring.
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- Publications of the Astronomical Society of Japan, 2015, v. 67, n. 6, p. 1, doi. 10.1093/pasj/psv074
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- Article
How does a secular instability grow in a hyperaccretion flow?
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- Publications of the Astronomical Society of Japan, 2015, v. 67, n. 5, p. 101-1, doi. 10.1093/pasj/psv070
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Radiation hydrodynamic instability in a plane-parallel, super-Eddington atmosphere: A mechanism for clump formation.
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- Publications of the Astronomical Society of Japan, 2014, v. 66, n. 2, p. 1, doi. 10.1093/pasj/psu011
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- Article
Diverse Polarimetric Features of AGN Jets from Various Viewing Angles: Towards a Unified View.
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- Galaxies (2075-4434), 2022, v. 10, n. 5, p. N.PAG, doi. 10.3390/galaxies10050103
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- Article
Black hole accretion: theoretical limits and observational implications.
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- Proceedings of the International Astronomical Union, 2006, v. 2, n. S238, p. 153, doi. 10.1017/S1743921307004887
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- Article