Shu-ichiro Inutsuka mainly investigates Astrophysics, Magnetohydrodynamics, Molecular cloud, Protostar and Interstellar medium. His Astrophysics study frequently draws parallels with other fields, such as Astronomy. His Magnetorotational instability study, which is part of a larger body of work in Magnetohydrodynamics, is frequently linked to Magnetic pressure, bridging the gap between disciplines.
His research in Molecular cloud intersects with topics in Molecular physics, Fragmentation and Isothermal process. He combines subjects such as Gravitational collapse, Spectral energy distribution, Field line and Angular momentum with his study of Protostar. Shu-ichiro Inutsuka focuses mostly in the field of Interstellar medium, narrowing it down to matters related to Shock wave and, in some cases, Supernova and Interstellar cloud.
Shu-ichiro Inutsuka mainly investigates Astrophysics, Molecular cloud, Star formation, Astronomy and Magnetohydrodynamics. Shu-ichiro Inutsuka regularly links together related areas like Turbulence in his Astrophysics studies. His Molecular cloud research integrates issues from Gravitational collapse, Shock wave, Supernova and Angular momentum.
Shu-ichiro Inutsuka has researched Star formation in several fields, including Fragmentation and Redshift. His work on Magnetorotational instability as part of general Magnetohydrodynamics study is frequently linked to Magnetic pressure, bridging the gap between disciplines. His studies in Protostar integrate themes in fields like Accretion and Outflow.
His scientific interests lie mostly in Astrophysics, Molecular cloud, Star formation, Stars and Interstellar medium. His Astrophysics research incorporates themes from Turbulence and Outflow. His work deals with themes such as Shock wave, Magnetohydrodynamics and Mass fraction, which intersect with Turbulence.
Shu-ichiro Inutsuka has included themes like Eddy current brake and Ohm's law in his Magnetohydrodynamics study. His research in Molecular cloud intersects with topics in Supernova remnant, Cosmic ray, Gravitational collapse, Line-of-sight and Millimeter. His Star formation study incorporates themes from Spectral line, Continuum and Redshift.
His primary areas of study are Astrophysics, Molecular cloud, Star formation, James Clerk Maxwell Telescope and Stars. His study connects Turbulence and Astrophysics. Shu-ichiro Inutsuka interconnects Continuum, Infrared, Outflow, Submillimeter Array and Protoplanetary disk in the investigation of issues within Molecular cloud.
Shu-ichiro Inutsuka combines subjects such as Planetary science, Fragmentation and Interstellar medium with his study of Star formation. His Interstellar medium study deals with Thermal intersecting with Magnetohydrodynamics, Gravitation and Virial theorem. His work on Small Magellanic Cloud as part of his general Stars study is frequently connected to Type, thereby bridging the divide between different branches of science.
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A Radiation Hydrodynamic Model for Protostellar Collapse. II. The Second Collapse and the Birth of a Protostar
Hirohiko Masunaga;Shu-ichiro Inutsuka.
The Astrophysical Journal (2000)
Angular Momentum Transport by MHD Turbulence in Accretion Disks: Gas Pressure Dependence of the Saturation Level of the Magnetorotational Instability
Takayoshi Sano;Shu-ichiro Inutsuka;Neal J. Turner;James M. Stone.
arXiv: Astrophysics (2003)
Discovery of Small-Scale Spiral Structures in the Disk of SAO 206462 (HD 135344B): Implications for the Physical State of the Disk from Spiral Density Wave Theory
T. Muto;T. Muto;C. A. Grady;J. Hashimoto;M. Fukagawa.
The Astrophysical Journal (2012)
An Origin of Supersonic Motions in Interstellar Clouds
Hiroshi Koyama;Shu-ichiro Inutsuka.
The Astrophysical Journal (2001)
Disk Winds Driven by Magnetorotational Instability and Dispersal of Proto-Planetary Disks
T. K. Suzuki;S. Inutsuka.
arXiv: Astrophysics (2008)
Making the corona and the fast solar wind: a self-consistent simulation for the low-frequency Alfven waves from photosphere to 0.3AU
Takeru K. Suzuki;Shu-ichiro Inutsuka.
arXiv: Astrophysics (2005)
Self-similar Solutions and the Stability of Collapsing Isothermal Filaments
Shu-Ichiro Inutsuka;Shoken M. Miyama.
The Astrophysical Journal (1992)
A Radiation Hydrodynamic Model for Protostellar Collapse. I. The First Collapse
Hirohiko Masunaga;Shoken M. Miyama;Shu-ichiro Inutsuka.
The Astrophysical Journal (1998)
A Production Mechanism for Clusters of Dense Cores
Shu-ichiro Inutsuka;Shoken M. Miyama.
The Astrophysical Journal (1997)
ANGULAR MOMENTUM TRANSPORT BY MAGNETOHYDRODYNAMIC TURBULENCE IN ACCRETION DISKS: GAS PRESSURE DEPENDENCE OF THE SATURATION LEVEL OF THE MAGNETOROTATIONAL INSTABILITY
Takayoshi Sano;Takayoshi Sano;Shu-ichiro Inutsuka;Neal J. Turner;Neal J. Turner;James M. Stone;James M. Stone.
The Astrophysical Journal (2004)
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