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| 書誌情報 | ファイル |
|---|---|
| How much can 56Ni be synthesized by the magnetar model for long gamma-ray bursts and hypernovae? Suwa, Y.; Tominaga, N. (2015-05-22) Monthly Notices of the Royal Astronomical Society, 451(1): 282-287 |  |
| THREE-DIMENSIONAL BOLTZMANN HYDRO CODE FOR CORE COLLAPSE IN MASSIVE STARS. I. SPECIAL RELATIVISTIC TREATMENTS Nagakura, Hiroki; Sumiyoshi, Kohsuke; Yamada, Shoichi (2014-10-01) The Astrophysical Journal Supplement Series, 214(2) | |
| From supernovae to neutron stars Suwa, Yudai (2014-03-28) Publications of the Astronomical Society of Japan, 66(2) | |
| Simulations of Core-collapse Supernovae in Spatial Axisymmetry with Full Boltzmann Neutrino Transport Nagakura, Hiroki; Iwakami, Wakana; Furusawa, Shun; Okawa, Hirotada; Harada, Akira; Sumiyoshi, Kohsuke; Yamada, Shoichi; Matsufuru, Hideo; Imakura, Akira (2018-02-20) The Astrophysical Journal, 854(2) | |
| EOSDB: The database for nuclear equations of state Ishizuka, Chikako; Suda, Takuma; Suzuki, Hideyuki; Ohnishi, Akira; Sumiyoshi, Kohsuke; Toki, Hiroshi (2015-01-20) Publications of the Astronomical Society of Japan, 67(1) | |
| Type Ic core-collapse supernova explosions evolved from very massive stars Yoshida, T.; Okita, S.; Umeda, H. (2014-02-18) Monthly Notices of the Royal Astronomical Society, 438(4): 3119-3127 | |
| The spectrum of a fast shock breakout from a stellar wind Ioka, Kunihito; Levinson, Amir; Nakar, Ehud (2019-04) Monthly Notices of the Royal Astronomical Society, 484(3): 3502-3509 | |