Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientist
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
Scientist
Univ.Tokyo
University of Tokyo
Univ. of Tokyo
Univ. Tokyo
Grad. School of Arts and Sciences, Univ. of Tokyo
U.Tokyo
Department of Earth Science and Astronomy, College of Arts and Sciences, University of Tokyo, Komaba, Meguro, Tokyo 153, Japan
University of Tokyo, Meguro, Tokyo, Japan
Tokyo, University, Japan
Department of Earth Science and Astronomy, Graduate School of Arts and Sciences, University of Tokyo Komaba, Meguro-ku, Tokyo 153-8902, Japan of Earth Science and Astronomy, Graduate School of Arts and Sciences, University of Tokyo, Komaba, Meguro, Tokyo 153, Japan
Department of Earth Science and Astronomy, Graduate School of Arts and Sciences, University of Tokyo, Komaba, Meguro, Tokyo 153-8902, Japan School of Arts and Science, The University of Tokyo, Komaba, Meguro, Tokyo 153-8902, Japan
Department of Earth Science and Astronomy, Graduate School of Arts and Sciences, University of Tokyo, Komaba, Meguro, Tokyo 153-8902, Japan
Department of Earth Science and Astronomy, Graduate School of Arts and Sciences, University of Tokyo, Komaba, Meguro, Tokyo 153-8902, Japan of Earth Science and Astronomy, Graduate School of Arts and Sciences, University of Tokyo, Komaba, Meguro-ku, Tokyo 153-8902, Japan of Earth Science and Astronomy, Graduate School of Arts and Sciences, University of Tokyo, 3-8-1 Komaba, Meguro, Tokyo 153-8902, Japan of Earth Science and Astronomy, Graduate School of Arts and Sciences, University of Tokyo, 3-8-1 Komaba, Meguro-ku, Tokyo 153-8902, Japan
University of Tokyo, Tokyo, Japan
univ. of Tokyo
Tokyo, University, Tokyo, Japan
Department of Earth Science & Astronomy, College
A criterion for the fragmentation of a rotating and collapsing gas cloud
A First Black Hole Imager, Caravan-sub at Andes
A general computational method for obtaining equilibria of self-gravitating and rotating gases
A general relativistic toroid around a black hole
A new numerical method for constructing quasi-equilibrium sequences of irrotational binary neutron stars in general relativity
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