Shu-ichiro Inutsuka

Professor

Nagoya University

Japan

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About

Shu-ichiro Inutsuka is a Professor at Nagoya University in Japan. His research areas encompass the growth and dynamics of molecular clouds, protoplanetary disks, and the formation of planetesimals, as evidenced by his recent publications. He has contributed to understanding mechanisms such as ambipolar diffusion, gravitational instability, and the energetic events affecting protoplanetary atmospheres.

Articles (16)

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2024

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2023

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2023

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2023

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2023

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2023

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2023

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2023

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2022

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2022

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2021

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2020

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2020

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2020

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2020

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2020

Collaborators (18)

Yasuhiro Oba

Associate Professor

JAPAN

Shu-ichiro Inutsuka

Research Interests

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Articles (16)

Growth of Massive Molecular Cloud Filament by Accretion Flows. I. Slow-shock Instability versus Ambipolar Diffusion

JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334

Triple Spiral Arms of a Triple Protostar System Imaged in Molecular Lines

Giant Impact Events for Protoplanets: Energetics of Atmospheric Erosion by Head-on Collision

On Secular Gravitational Instability in Vertically Stratified Disks

An Origin of Narrow Extended Structure in the Interstellar Medium: An Interstellar Contrail Created by a Fast-moving Massive Object

Planetesimal Formation by the Gravitational Instability of Dust Ring Structures

Evolution of the Angular Momentum of Molecular Cloud Cores Formed from Filament Fragmentation

Nonlinear Outcome of Coagulation Instability in Protoplanetary Disks. II. Dust-ring Formation Mediated by Backreaction and Fragmentation

Nonlinear Outcome of Coagulation Instability in Protoplanetary Disks. I. First Numerical Study of Accelerated Dust Growth and Dust Concentration at Outer Radii

FAUST. II. Discovery of a Secondary Outflow in IRAS 15398−3359: Variability in Outflow Direction during the Earliest Stage of Star Formation?

ALMA CO Observations of the Gamma-Ray Supernova Remnant RX J1713.7–3946: Discovery of Shocked Molecular Cloudlets and Filaments at 0.01 pc Scales

Bimodal Behavior and Convergence Requirement in Macroscopic Properties of the Multiphase Interstellar Medium Formed by Atomic Converging Flows

Secular Gravitational Instability of Drifting Dust in Protoplanetary Disks: Formation of Dusty Rings without Significant Gas Substructures

Early Evolution of Disk, Outflow, and Magnetic Field of Young Stellar Objects: Impact of Dust Model

Dispersal of protoplanetary discs by the combination of magnetically driven and photoevaporative winds

Collaborators (18)

Yasuhiro Oba

Hidekazu Tanaka

Jaehan Bae

Tsuyoshi Inoue

Tomoaki Matsumoto

Tetsuo Hasegawa

Takahiro Hayakawa

Timothy M. Gledhill

Kenji Kurosaki

Seokho Lee

Pierre Bastien

Tetsuya Hama

Francisca Kemper

Eun Jung Chung

Nigel Maxted

Ryo Yamazaki

Takaaki Tanaka

Yoko Oya

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