399 citations · 10.7k across the 204 of their papers we have counts for
206 papers
Application and Evaluation of the Material Point Method for Low-Velocity Asteroid Collisions Involving Large Deformations
Haru Fukuta, Tomoaki Ishiyama, Shu-ichiro Inutsuka
The collisional lifetimes of asteroids larger than km in the present-day main belt are estimated to exceed the age of the solar system, suggesting that their shapes may p…
The Milky Way Atlas for Linear Filaments III: Giant filaments and magnetic fields as evidence of a bubbly Galactic disk
Naval K. Bhadari, Ke Wang, Shu-ichiro Inutsuka +1
Linear filamentary structures are fundamental constituents of the interstellar medium and play a central role in star formation. Their relative orientation with respect to the ambi…
Formation of Isotopically Heterogeneous Molecular Cloud Cores in Filamentary Molecular Clouds
Yoshiaki Misugi, Shu-ichiro Inutsuka, Taishi Nakamoto +1
Meteorite analysis shows that the older solids of the solar system, such as the calcium-aluminum-rich inclusions (CAIs), have isotopic inhomogeneity. This indicates that the isotop…
From inter-filamentary gas to filaments and hubs: gas flows in the Mon R2 hub-filament system
Jihye Hwang, Doris Arzoumanian, Yoshito Shimajiri +5
Hub-filament systems (HFSs) play an important role in the formation of massive stars and star clusters. Although the velocity structures along dense filaments have been studied, th…
Modeling the Accretion of High-Velocity Clouds from a Rotating Halo
Izumi Seno, Shu-ichiro Inutsuka, Jiro Shimoda
High-Velocity Clouds (HVCs) are a major fuel reservoir for star formation in the Galactic disk. Determining their origin and kinematics is thus crucial for understanding Galactic e…
An Origin of Radially Aligned Filaments in Hub-Filament Systems
Shingo Nozaki, Shu-ichiro Inutsuka
Recent observations have identified hub-filament systems (HFSs) as the primary formation sites of massive stars and star clusters. Some HFSs are characterized by multiple filaments…