Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Kyoto University
YITP, Kyoto University
Univ. of Tokyo
Yukawa Institute for Theoretical Physics, Kyoto University
Yukawa Institute for Theoretical Physics, Kyoto University, Oiwake-cho Kitashirakawa Sakyo-ku, Kyoto 606-8502, Japan
Yukawa Institute for Theoretical Physics, Kyoto University, Oiwake-cho, Kitashirakawa, Sakyo-ku, Kyoto, 606-8502, Japan of Physics, School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan; Research Center for the Early Universe, School of Science, the University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan. Institute for Theoretical Physics, Sakyo-ku, Kyoto 606-8502, Japan
Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan
Yukawa Institute for Theoretical Physics, Kyoto University, Kitashirakawa-Oiwake-cho, Sakyo-ku, Kyoto 606-8502
Yukawa Institute for Theoretical Physics, Kyoto University;, KIPAC, Stanford University
Yukawa Institute for Theoretical Physics, Kyoto University, Oiwakecho, Kitashirakawa, Sakyoku, Kyoto 606-8502, Japan nagatakiatyukawa.kyoto-u.ac.jp
Yukawa Institute for Theoretical Physics, Kyoto University, Oiwakecho, Kitashirakawa, Sakyoku, Kyoto 606-8502, Japannagatakiatyukawa.kyoto-u.ac.jp nagatakiatyukawa.kyoto-u.ac.jp
Department of Physics, University of Tokyo; Research Center for the Early Universe, University of Tokyo.
Theoretical Astrophysics Group, Tokyo, 113-0033, Japan, tokyo.ac.jp Institute for Theoretical Physics, Kyoto University, Sakyo, Kyoto, Japan
Department of Physics, School of Science, the University of Tokyo, Tokyo 113, Japan
Department of Physics, School of Science, the
3-D Numerical Simulations of the Binary System PSR B1259-63/SS 2883 and High Energy Emission from the Disk-Wind Interaction Region
A Generalized Model of Nonlinear Diffusive Shock Acceleration Coupled to an Evolving Supernova Remnant
A high-frequency study of the Sunyaev-Zel'dovich effect morphology in galaxy clusters
A New Method for Calculating Arrival Distribution of Ultra-High Energy Cosmic Rays above 10^19 eV with Modifications by the Galactic Magnetic Field
A peculiar jet and arc of molecular gas toward the rich and young stellar cluster Westerlund 2 and a TeV gamma ray source
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