399 citations · 10.7k across the 204 of their papers we have counts for
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Emergence of Protoplanetary Disks and Successive Formation of Gaseous Planets by Gravitational Instability
Shu-ichiro Inutsuka, Masahiro N. Machida, Tomoaki Matsumoto
We use resistive magnetohydrodynamical simulations with the nested grid technique to study the formation of protoplanetary disks around protostars from molecular cloud cores that p…
Protoplanetary Disk Winds by Magnetorotational Instability : Formation of an Inner Hole and a Crucial Assist for Planet Formation
Takeru K. Suzuki, Takayuki Muto, Shu-ichiro Inutsuka
By constructing a global model based on 3D local magnetohydrodynamical (MHD) simulations, we show that the disk wind driven by magnetorotational instability (MRI) plays a significa…
Two-Fluid MHD Simulations of Converging Hi Flows in the Interstellar Medium. II: Are Molecular Clouds Generated Directly from Warm Neutral Medium?
Tsuyoshi Inoue, Shu-ichiro Inutsuka
Formation of interstellar clouds as a consequence of thermal instability is studied using two-dimensional two-fluid magnetohydrodynamic simulations. We consider the situation of co…
N-Body Simulation of Planetesimal Formation through Gravitational Instability and Coagulation. II. Accretion Model
Shugo Michikoshi, Eiichiro Kokubo, Shu-ichiro Inutsuka
The gravitational instability of a dust layer is one of the scenarios for planetesimal formation. If the density of a dust layer becomes sufficiently high as a result of the sedime…
Emission from a Young Protostellar Object I. Signatures of Young Embedded Outflows
M. Yamada, M. N. Machida, S. Inutsuka +1
We examine emission from a young protostellar object (YPO) with three-dimensional ideal MHD simulations and three-dimensional non-local thermodynamic equilibrium (non-LTE) line tra…
Protostellar Jet and Outflow in the Collapsing Cloud Core
Masahiro N. Machida, Shu-ichiro Inutsuka, Tomoaki Matsumoto
We investigate the driving mechanism of outflows and jets in star formation process using resistive MHD nested grid simulations. We found two distinct flows in the collapsing cloud…