His primary scientific interests are in Astrophysics, Accretion, Black hole, Astronomy and Active galactic nucleus. His study brings together the fields of Radiative transfer and Astrophysics. His Accretion research includes elements of Thin disk and Compton scattering, Electron.
The study incorporates disciplines such as Stellar mass, Plasma, Radiative cooling and Accretion disc in addition to Black hole. Shin Mineshige works mostly in the field of Astronomy, limiting it down to topics relating to Gamma-ray astronomy and, in certain cases, Observatory, Spectrometer, Imaging spectrometer, Angular resolution and Detector, as a part of the same area of interest. In his study, Cauchy stress tensor and Gravitational energy is strongly linked to Spectral index, which falls under the umbrella field of Active galactic nucleus.
The scientist’s investigation covers issues in Astrophysics, Accretion, Astronomy, Black hole and Accretion disc. Shin Mineshige interconnects Spectral line and Radiative transfer in the investigation of issues within Astrophysics. His Accretion research integrates issues from Thin disk, Radiation, Corona and Compton scattering.
His Instability research extends to Astronomy, which is thematically connected. In his study, which falls under the umbrella issue of Black hole, Effective temperature is strongly linked to Radius. His study in Light curve is interdisciplinary in nature, drawing from both Quasar and Gravitational microlensing.
His primary areas of study are Astrophysics, Accretion, Line, Radiative transfer and Spectral line. His work focuses on many connections between Astrophysics and other disciplines, such as Photon, that overlap with his field of interest in Pulsar. His research integrates issues of Radiation, Compton scattering, Accretion disc and Instability in his study of Accretion.
His Line study integrates concerns from other disciplines, such as Spectral resolution, Ionization and Emission spectrum. His research in Radiative transfer intersects with topics in Gravitation and Computational physics. His work carried out in the field of Black hole brings together such families of science as Radius, Luminosity, Circular orbit and Light curve.
His scientific interests lie mostly in Astrophysics, Astronomy, Emission spectrum, Accretion and Ionization. Eddington luminosity, Active galactic nucleus, Galaxy, Intracluster medium and Pulsar are subfields of Astrophysics in which his conducts study. His Eddington luminosity course of study focuses on Schwarzschild radius and Convection, Photon energy and Spectral line.
Many of his research projects under Astronomy are closely connected to Feature and High resolution with Feature and High resolution, tying the diverse disciplines of science together. In most of his Accretion studies, his work intersects topics such as Radiation. As a part of the same scientific family, he mostly works in the field of Radiation, focusing on Inflow rate and, on occasion, Black hole.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
Black-hole accretion disks
Shoji Kato;Jun Fukue;Shin Mineshige.
Black-hole accretion disks. Edited by Shoji Kato (1998)
Black-Hole Accretion Disks --- Towards a New Paradigm ---
S. Kato;J. Fukue;S. Mineshige.
Black-Hole Accretion Disks --- Towards a New Paradigm (2008)
Supercritical Accretion Flows around Black Holes: Two-dimensional, Radiation Pressure-dominated Disks with Photon Trapping
Ken Ohsuga;Ken Ohsuga;Masao Mori;Masao Mori;Taishi Nakamoto;Shin Mineshige.
The Astrophysical Journal (2005)
Super-critical Accretion Flows around Black Holes: Two-dimensional, Radiation-pressure-dominated Disks with Photon-trapping
K. Ohsuga;M. Mori;T. Nakamoto;S. Mineshige.
arXiv: Astrophysics (2005)
GLOBAL STRUCTURE OF THREE DISTINCT ACCRETION FLOWS AND OUTFLOWS AROUND BLACK HOLES FROM TWO-DIMENSIONAL RADIATION-MAGNETOHYDRODYNAMIC SIMULATIONS
Ken Ohsuga;Shin Mineshige.
The Astrophysical Journal (2011)
Global Structure of Three Distinct Accretion Flows and Outflows around Black Holes through Two-Dimensional Radiation-Magnetohydrodynamic Simulations
Ken Ohsuga;Shin Mineshige.
arXiv: High Energy Astrophysical Phenomena (2011)
The quiescent intracluster medium in the core of the Perseus cluster
Felix Aharonian;Felix Aharonian;Hiroki Akamatsu;Fumie Akimoto;Steven W. Allen.
(2016)
Slim-Disk model for Soft X-Ray Excess and Variability of Narrow-Line Seyfert 1 Galaxies
Shin Mineshige;Toshihiro Kawaguchi;Mitsuru Takeuchi;Kiyoshi Hayashida.
Publications of the Astronomical Society of Japan (2000)
Galactic Black-Hole Candidates Shining at the Eddington Luminosity
Ken-ya Watarai;Jun Fukue;Mitsuru Takeuchi;Shin Mineshige.
Publications of the Astronomical Society of Japan (2000)
Global Radiation-Magnetohydrodynamic Simulations of Black-Hole Accretion Flow and Outflow: Unified Model of Three States
Ken Ohsuga;Shin Mineshige;Masao Mori;Yoshiaki Kato.
Publications of the Astronomical Society of Japan (2009)
If you think any of the details on this page are incorrect, let us know.
We appreciate your kind effort to assist us to improve this page, it would be helpful providing us with as much detail as possible in the text box below:
Masaryk University
Netherlands Institute for Space Research
Dublin Institute For Advanced Studies
Stanford University
Durham University
University of Michigan–Ann Arbor
Kyoto University
University of Southampton
Space Telescope Science Institute
Stanford University
Lancaster University
University of Montana
Kyoto Pharmaceutical University
University of South Carolina
Duke University
Fujian Normal University
Huazhong Agricultural University
Northeastern University
Oregon State University
University of Pennsylvania
Leiden University Medical Center
Norwegian Meteorological Institute
Nagoya University
Mayo Clinic
University of Connecticut
Lancaster University