Mathematics – Rings and Algebras
Scientist
Mathematics
Rings and Algebras
Scientist
CrAO
IoA, U. Tokyo
UTokyo, MAGNUM
Tokyo, Japan
Institute of Astonomy, University of Tokyo
IOA, Tokyo
Univ. of Tokyo
Tokyo Astronomical Observatory, Mitaka, Japan
Mount Stromlo and Siding Spring Observatoires, Canberra, Australia
Tohoku University, Sendai, Japan
Institute of Astronomy, School of Science, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan; Research Center for the Early Universe, School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
Durham, University, England; Copenhagen, University, Denmark
IOA, Japan
Institute of Astronomy, School of Science, University of Tokyo, Mitaka, Tokyo 181-0015, Japan; Research Center for the Early Universe, School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
Institute of Astronomy, Faculty of Science, University of Tokyo, Mitaka, Tokyo 181, Japan
Research Center for the Early Universe, Faculty of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
Institute of Astronomy, University of Tokyo
National Astronomical Observatory, Mitaka, Japan
IofA, Tokyo University
Institute of Astronomy, School of Science, University of Tokyo, 2-21-1 Osawa, Mitaka-shi, Tokyo 181-0015, Japan; Research Center for the Early Universe, School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
Tokyo Astronomical Observatory, Tokyo, Japan
University of Tokyo, Japan
Durham, University, England; National Astronomical Observatory, Mitaka, Japan
Research Center for the Early Universe, School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan; Institute of Astronomy, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan.
A fragmentation-coalescence model for the initial stellar mass function
A hydrodynamic interaction between the galactic disk and halo, and its application to the origin of warping gaseous disks
A Revised Broad-Line Region Radius and Black Hole Mass for the Narrow-Line Seyfert 1 NGC 4051
A Two-Component Model for the Light Curves of Hypernovae
Abundance gradients in the star-forming viscous disk and chemical properties of the bulge.
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