Explosion Geometry of a Rotating 13M_⨀ Star Driven by the SASI-Aided Neutrino-Heating Supernova Mechanism
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概要
- 論文の詳細を見る
- 2010-12-25
著者
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KOTAKE Kei
Division of Theoretical Astronomy National Astronomical Observatory of Japan
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Liebendorfer Matthias
Department Of Physics University Of Basel
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Sato Katsuhiko
The Institute For The Physics And Mathematics Of The Universe The University Of Tokyo
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Suwa Yudai
Department Of Physics School Of Science The University Of Tokyo
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Whitehouse Stuart
Department Of Physics University Of Basel
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TAKIWAKI Tomoya
Center for Computational Astrophysics, National Astronomical Observatory of Japan
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Takiwaki Tomoya
Center For Computational Astrophysics National Astronomical Observatory Of Japan
関連論文
- Explosive Nucleosynthesis in Magnetohydrodynamical Jets from Collapsars(Astrophysics and Cosmology)
- Explosion Geometry of a Rotating 13M_⨀ Star Driven by the SASI-Aided Neutrino-Heating Supernova Mechanism
- Magnetorotational Collapse of Population III Stars
- Explosive Nucleosynthesis in Magnetohydrodynamical Jets from Collapsars. II : Heavy-Element Nucleosynthesis of s, p, r-Processes(Astrophysics and Cosmology)
- Explosive Nucleosynthesis in Magnetohydrodynamical Jets from Collapsars