Specifying the Environments around GRB, Explaining the Fe Line in the X-Ray Afterglow of GRB 000214
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概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 2001-08-25
著者
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Nagataki Shigehiro
Department Of Physics School Of Science The University Of Tokyo
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Nagataki Shigehiro
Department Of Phisics University Of Tokyo
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KOTAKE Kei
Department of Physics, School of Science, The University of Tokyo
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Kotake Kei
Department Of Physics School Of Science The University Of Tokyo
関連論文
- Nonrelativistic and Relativistic Treatments for Propagation of Torsional Resonant Alfven Waves in Strongly Magnetized Neutron Stars(Astrophysics and Relativity)
- Pulsar Kick and Asymmetric Iron Velocity Distribution in SN 1987A
- Revision of the Selection Function of the Optical Redshift Survey Using the Sloan Digital Sky Survey Early Data Release : Toward an Accurate Estimate of the Source Number Density of Ultra-High Energy Cosmic Rays
- Propagation of Ultra-High Energy Cosmic Rays from Sources in the Super-Galactic Plane
- Chemical Evolution in the Large Magellanic Cloud
- Implications of the Discovery of a Millisecond Pulsar in SN 1987A
- Initial Shock Waves for Explosive Nucleosynthesis in Type II Supernova
- The r-Process Nucleosynthesis in Neutrino-/Magnetocentrifugally-Driven Winds
- Features of Neutrino Signals from Collapsars
- Specifying the Environments around GRB, Explaining the Fe Line in the X-Ray Afterglow of GRB 000214
- Dispersion of Inferred SNe Ia/SNe II Ratios for Current Models of Supernova Nucleosynthesis