Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Keio Univ.
Keio University
Kieo Univ.
Keio U.
Department of Astronomy, Keio University, Yokohama 223-8521, Japan
Pennsylvania State University, University Park
Department of Earth and Planetary Science, Tokyo Institute of Technology, Ookayama 2-1-12-I2-10, Meguro-ku, Tokyo, Japan of Astronomy, Keio University, 4-1-1 Hiyoshi, Kohoku, Yokohama, Kanagawa 223-8521, Japan
Department of Astronomy, Keio University, Kouhoku-ku, Yokohama 223-8521
Department of Astronomy, Keio University, Hiyoshi, Kouhoku-ku, Yokohama 223-8521, Japan
Tokyo Institute of Technology, Japan
Keio University, Yokohama, Japan; Illinois, University, Urbana
Keio University, Tokyo, Japan
Illinois, University, Urbana; Pennsylvania State University, University Park
Pennsylvania State University, University Park; Illinois, University, Urbana
Keio Univ., Hiyoshi, Japan
Keio University, Yokohama, Japan
Kyowa Interface Science Co., Ltd., Japan
Kyowa Interface Science Co., Ltd., Saitama, Japan
Inst. of Physics, Univ. of Tokyo
Graduate School of Human and Environmental Studies, Kyoto University, Kyoto 606-8501, Japan
Sagamihara, Japan
Nagoya University, Furo-cho, Chikusa-ku, Nagoya, 464-8602, Japan
Department of Earth and Planetary Sciences, Nagoya University Nagoya 464-01, Japan
Tokyo, University, Tokyo, Japan
Nagoya University, Nagoya, Japan
Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, USA
Department of Geophysics, Kyoto University, Kyoto 606-8502, Science Group, Graduate School of Human and Environmental Studies, Kyoto University, Kyoto 606-8501, Japan
Earth Remote Sensing Data Analysis Center, 3-12-1 Kachidoki, Chuo-ku, Tokyo, 104-0054 Japan
Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institut
1/8 anomaly in the excess-oxygen-doped La_1.8_Nd_0.2_Cu_1-y_Zn_y_O_4+δ_
59Co, 23Na, and 1H NMR Studies of Double-Layer Hydrated Superconductors NaxCoO2-yH2O
A Light-Curve Model of the Symbiotic Nova PU Vul (1979) -- A Very Quiet Explosion with Long-Lasted Flat Peak
A limit cycle model for long-term optical variations of V Sagittae: The second example of accretion wind evolution
A Model for the Quiescent Phase of the Recurrent Nova U Scorpii
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