399 citations · 10.7k across the 204 of their papers we have counts for
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Secular Gravitational Instability of a Dust Layer in Shear Turbulence
Shugo Michikoshi, Eiichiro Kokubo, Shu-ichiro Inutsuka
We perform a linear stability analysis of a dust layer in a turbulent gas disk. Youdin (2011) investigated the secular gravitational instability of a dust layer using hydrodynamic…
A Detailed Study of the Molecular and Atomic Gas Toward the γ-ray SNR RX J1713.7-3946: Spatial TeV γ-ray and ISM Gas Correspondence
Y. Fukui, H. Sano, J. Sato +14
RX J1713.73946 is the most remarkable TeV -ray SNR which emits -rays in the highest energy range. We made a new combined analysis of CO and \ion{H}{1} in the SNR and deriv…
A Fast and Accurate Calculation Scheme for Ionization Degrees in Protoplanetary and Circumplanetary Disks with Charged Dust Grains
Yuri I. Fujii, Satoshi Okuzumi, Shu-ichiro Inutsuka
We develop a fast and accurate calculation method for ionization degrees in protoplanetary and circumplanetary disks including dust grains. We apply our method to calculate the ion…
Toward Understanding the Cosmic-ray Acceleration at Young Supernova Remnants Interacting with Interstellar Clouds: Possible Applications to RX J1713.7-3946
Tsuyoshi Inoue, Ryo Yamazaki, Shu-ichiro Inutsuka +1
Using three-dimensional magnetohydrodynamics simulations, we investigate general properties of a blast wave shock interacting with interstellar clouds. The shock-cloud interaction…
Gravitational Fragmentation of Expanding Shells. II. Three-dimensional Simulations
Kazunari Iwasaki, Shu-ichiro Inutsuka, Toru Tsuribe
We investigate the gravitational fragmentation of expanding shells driven by HII regions using the three-dimensional Lagrangian simulation codes based on the Riemann solver, called…
Gravitational Fragmentation of Expanding Shells. I. Linear Analysis
Kazunari Iwasaki, Shu-ichiro Inutsuka, Toru Tsuribe
We perform a linear perturbation analysis of expanding shells driven by expansions of HII regions. The ambient gas is assumed to be uniform. As an unperturbed state, we develop a s…