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Shin Mineshige

Kyoto University
Yukawa Institute for Theoretical Physics

500

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Striking similarities in mean shot profiles of the black hole binary Cyg X-1, the blazar W2R 1926+42, and the cataclysmic variable MV Lyr

2021
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Variability of Comptonized X-ray spectra of a super-Eddington accretor: Approach using Boltzmann radiation transport

2021 Publications of the Astronomical Society of Japan
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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

2021 Publications of the Astronomical Society of Japan
- Norita Kawanaka
- Shin Mineshige
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The origins and impact of outflow from super-Eddington flow

2021 Publications of the Astronomical Society of Japan
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Outflow from super-Eddington flow: where it originates from and how much impact it gives?.

2021 arXiv: High Energy Astrophysical Phenomena
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Polarization images of accretion flow around supermassive black holes: imprints of toroidal field structure

2021 Publications of the Astronomical Society of Japan
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Molecular clouds under the FUV feedback: factories of CO-dark gas

2020 arXiv: Astrophysics of Galaxies
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Polarization images of accretion flow around supermassive black holes: imprints of toroidal field structure

2020 arXiv: High Energy Astrophysical Phenomena
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Factories of CO-dark gas: molecular clouds with limited star formation efficiencies by far-ultraviolet feedback

2020 Monthly Notices of the Royal Astronomical Society
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What Determines Unique Spectra of Super-Eddington Accretors?: Origin of Optically Thick and Low Temperature Coronae in Super-Eddington Accretion Flows. (arXiv:2012.05386v1 [astro-ph.HE])

2020
- Norita Kawanaka
- Shin Mineshige
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