Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
U. Tokyo, Japan
Department of Astronomy, Graduate School of Science, The University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-0033, Japan
Department of Astronomy School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
Department of physics, Konan University, 8-9-1 Okamoto, Kobe, Hyogo 658-8501, Japan; Institute for the Physics and Mathematics of the Universe, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan
Division of Optical and Infrared Astronomy, National Astronomical Observatory of Japan, Mitaka, Tokyo, Japan
Department of Astronomy, School of Science, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
Department of Physics, Faculty of Science and Engineering, Konan University, 8-9-1 Okamoto, Kobe, Hyogo 658-8501, Japan; Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwanoha 5-1-5, Kashiwa, Chiba 277-8583, Japan
Department of Physics, Faculty of Science and Engineering, Konan University, 8-9-1 Okamoto, Kobe, Hyogo 658-8501, Japan and Institute for the Physics and Mathematics of the Universe, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8569, Japan tominagaatkonan-u.ac.jp
Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwa, Chiba 277-8583, Japan; Department of Physics, Faculty of Science and Engineering, Konan University, 8-9-1 Okamoto, Kobe, Hyogo 658-8501, Japan
Department of Astronomy, School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan of Astronomy, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
University of Tokyo
Department of Astronomy, School of Scienece, University of Tokyo, Tokyo, 113-0033, Japan of Astronomy, University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-0033, Japan
University of Tokyo, Japan
3D Signatures of off-center Delayed-Detonation Models
A Core-Collapse Supernova Model for the Extremely Luminous Type Ic Supernova 2007bi: An Alternative to the Pair-Instability Supernova Model
A Hypernova Model for SN 2003dh/GRB 030329
A neutron-star-driven X-ray flash associated with supernova SN 2006aj
A very low upper limit for a Be abundance of a carbon-enhanced metal-poor star
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