Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Univ. of Tokyo
Research Center for the Early Universe, University of Tokyo
Tokyo, University, Japan
University of Tokyo, Tokyo, Japan
Research Center for the Early Universe, University of Tokyo, Tokyo, Japan
Graduate School of Science, University of Tokyo, Japan
Max-Planck-Institut für Astrophysik, Garching bei München, Germany
Research Center for the Early Universe, Graduate School of Science, University of Tokyo, Bunkyo-ku, Tokyo, 113-0033, Japan
Department of Astronomy, Graduate School of Science, University of Tokyo, Japan; Research Center for the Early Universe, Graduate School of Science, University of Tokyo, Japan
Max-Planck-Institut für Physik und Astrophysik, Garching bei München, Germany; Tokyo, University, Japan
The Institute of Physical and Chemical Research, Saitama, Japan
Department of Astronomy and Research Center for the Early Universe, School of Science, University of Tokyo, Tokyo 113, JapanHideakiTakabeInstitute of Laser Engineering, Osaka University, Suita, Osaka 565, Japan
Department of Astronomy, School of Science, The University of Tokyo, Bunkyo-ku, Tokyo 113
Department of Astronomy, Graduate School of Science, University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo, 113-0033 Japan; Research Center for the Early Universe, Graduate School of Science, University of Tokyo
Department of Astronomy, Graduate School of Science, University of Tokyo, Tokyo, Japan; Research Center for the Early Universe, Graduate School of Science, University of Tokyo, Tokyo, Japan
University of Tokyo
Research Center for the Early Universe, Graduate School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan Graduate School of Science, University of Tokyo, Tokyo, Japan
Research Center for the Early Universe, Graduate School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
Tokyo Univ., Japan
Tokyo, University, Japan; Max-Planck-Institut für Physik und Astrophysik, G
A conservative scheme for the relativistic Vlasov-Maxwell system
A Low Mass Helium Star Model for the Type Ic Supernova 1987M
A Merging Scenario for Globular Cluster Formation -- Inhibition or Promotion of Self-Enrichment
A method to identify the companion stars of type Ia supernovae in young supernova remnants
A Novel Method to Construct Stationary Solutions of the Vlasov Maxwell system
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