Evolution transition from rapidly rotating neutron stars to strange stars
スポンサーリンク
概要
著者
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Arai K
Kumamoto Univ. Kumamoto
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Hashimoto Masa-aki
Department Of Physics Kyushu University
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Hashimoto Masa-aki
Department Of Physics Faculty Of Science Kyusyu University
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Hashimoto Masa‐aki
Kyushu Univ. Fukuoka
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Hashimoto M
Department Of Physics Kyushu University
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Hashimoto Michio
Department Of Physics Nagoya University
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Hashimoto Masashi
Research Fellow Of The Japan Society For The Promotion Of Science
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Hashimoto Masa‐aki
Department Of Physics Kyushu University
関連論文
- Effects of a New Triple-α Reaction Rate on the Helium Ignition of Accreting White Dwarfs
- Global structure of an accretion disk with self-gravity
- Steady structure of advection dominated accretion disks with global magnetic fields
- Equilibrium structure of advection dominated accretion disks around black holes
- Explosive Nucleosynthesis in Magnetohydrodynamical Jets from Collapsars(Astrophysics and Cosmology)
- MHD simulations of a collapsar model
- Nuclear flashes toward superbursts in accreting neutron stars
- Exotic cooling on isolated neutron stars with different surface composition
- Effects of QCD phase transition on the collapse and bounce of a differentially rotating massive star
- Observational constrains on a decaying Λ cosmology