Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Kyoto Univ.
Kyoto-u, Japan
Kyoto University
Nagoya Univ.
Kyoto U.
NAO, Japan
Department of Physics, Kyoto University, Kyoto, 606-8502, Japan
NAO Japan
National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan; and Department of Physics, Kyoto University, Kyoto 606-8502, Japan
Department of Physics, Kyoto University, Kitashirakawa, Kyoto 606-8502, Japan of Physics, Kyoto University, Kitashirakawa, Sakyo, Kyoto 606-8502, Japan of Physics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8602, Japan
Department of Physics, Nagoya University, Nagoya 463-8602, Japan
Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan
Department of Physics, Kyoto University, Kyoto, Kyoto 606-8502, Japan and Department of Physics, Nagoya University, Nagoya, Aichi 464-8602, Japan
Department of Physics, Kyoto University, Kyoto, 606-8502, Japan & Department of Physics, Nagoya University, Nagoya, Aichi 464-8602, Japan
Department of Physics, Nagoya University
Division of Theoretical Astrophysics, National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan
Department of Physics, Graduate School of Science, Kyoto University, Sakyo-ku, Kyoto 606-8502, Japan Astronomical Observatory, Mitaka, Tokyo, 181-8588, Japan of Physics, Nagoya University, Chikusa-ku, Nagoya, Aichi 464-8602, Japan of Physics, Kyoto University, Kitashirakawa, Sakyo-ku, Kyoto 606-8502, Japan Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo 181-8588, Japan; Department of Physics, Kyoto University, Kyoto 606-8502, Japan.
Department of Physics, Kyoto University, Kitashirakawa-Oiwake-Cho, Sakyo-ku, Kyoto, 606-8502, JAPAN
National Astronomical Observatory, Mitaka, Japan
NAOJ
Nagoya University, J
$N$-body Simulation of Planetesimal Formation Through Gravitational Instability of a Dust Layer
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
A Fast and Accurate Calculation Scheme for Ionization Degrees in Protoplanetary and Circumplanetary Disks with Charged Dust Grains
A Fast Numerical Scheme for Causal Relativistic Hydrodynamics with Dissipation
A Hybrid Scenario for Planet Formation
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