Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Kyoto U
Kyoto Univ.
Hokkai-Gakuen University
Hida Observatory, Japan
Kyoto University
Universitäts-Sternwarte, Geismarlandstrasse 11, D-37083 Göttingen, Germany; Hida Observatory, Kyoto University, Kamitakara, Gifu 506-1314, Japan
Hida Observatory, Kyoto University, Kamitakara, Gifu, Japan
Department of Astronomy, Faculty of Science, Kyoto University, Sakyo-ku, Kyoto 606-8502, Japan Observatory, Kyoto University, Kamidakara, Gifu 506-1314
Hida Observatory, Kyoto University / Universitets-Sternwarte
Kwasan Observatory, Kyoto University, Yamashina-ku, Kyoto 607-8471, Japan
Hida Observatory, Kyoto University, Kamitakara, Gifu 506-1314
Hida Observatory, Kyoto University, Kamitakara, Gifu 506-1314, Japan
Universitäts-Sternwarte, Geismarlandstrasse 11, D-37083 Göttingen, Germany; Department of Astronomy, Faculty of Science, Kyoto University, Sakyo-ku, Kyoto 606-8502, Japan
Department of Astronomy, Faculty of Science, Kyoto University, Sakyo-ku, Kyoto 606-01
Department of Astronomy, Faculty of Science, Kyoto University, Sakyo-ku, Kyoto 606-8502, Japan; Universitäts-Sternwarte, Geismarlandstrasse 11, D-37083 Göttingen, Germany
Hida Observatory, Graduate School of Science, Kyoto University, Kamitakara, Gifu 506-1314
Department of Astronomy, Faculty of Science, Kyoto University, Sakyo-ku, Kyoto 606-8502
"Huruhata's Variable" Revealed: The WZ Sge-Type Dwarf Nova EG CANCRI
1998 Superoutburst of the Large-Amplitude SU UMa-Type Dwarf Nova WX Ceti
A Deep Dip during an Outburst in the Old Nova, Q Cygni
A Deeply Eclipsing SU UMa-Type Dwarf Nova with the Shortest Orbital Period, XZ Eridani
A New SU UMa-Type Dwarf Nova, QW Serpentis (= TmzV46)
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