Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Hokkaido Univ
Niigata University, Ikarashi, Japan; Illinois, University, Urbana, IL
Niigata University, Niigata, Japan
Hakkaido U., Japan
Department of Physics, Hokkaido University, Sapporo 060-0810, Japan
Division of Science, Hokkaido University, Sapporo 060-0810, Japan; Meme Media Laboratory, Hokkaido University, Sapporo 060-0813, Japan
Max-Planck-Institut für Physik und Astrophysik, Garching bei München, Germany
Tokyo, University, Tokyo, Japan
Department of Physics, Hokkaido University, Sapporo, Hokkaido 060-0810, Japan
Niigata University, Japan
Hokkaido Univ.
Hokkaido University
Graduate School of Science, Hokkaido University
Department of Physics, Hokkaido University, N-12 W-8 Kitaku, Sapporo 060-8810, Japan of Physics / Department of Cosmosciences, Hokkaido University, Kita 10, Nishi 8, Kita-ku, Sapporo 060-0810
Department of Physics, Hokkaido University, Sapporo 060-0810, Japan of Cosmosciences, Hokkaido University, Kita 10 Nishi 8, Kita-ku, Sapporo, 060-0810, Japan of Cosmoscience, Hokkaido University, Sapporo, Hokkaido 060-0810, Japan
Niigata Univ., Japan
Department of Physics, Faculty of Science, Hokkaido University, Sapporo, Hokkaido 060-0810, Japan
Niigata University, Niigata-shi, Japan
Department of Physics, Hokkaido University, Sapporo, Japan 060-0810
Graduate School of Science, Hokkaido University, Kita-ku, Sapporo 060-0810, Japan
Department of Physics, Hokkaido University, Sapporo, Hokkaido 060-0810, Japan University, Japan; Max-Planck-Institut für Astrophysik, Garching bei München, Ge
A Model of Deep Mixing in Globular Cluster Red Giants
A new model for s-process nucleosynthesis in low-mass, low-metallicity AGB stars
A Theory of Hydrogen Shell Flashes on Accreting White Dwarfs - Part Two - the Stable Shell Burning and the Recurrence Period of Shell Flashes
A theory of hydrogen shell flashes on accreting white dwarfs. I - Their progress and the expansion of the envelope. II - The stable shell burning and the recurrence period of shell flashes
An abundance study of the most iron-poor star HE1327-2326 with Subaru/HDS
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