X-Ray Afterglow from the Matter Heated by Emission of GRB(Poster)
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概要
- 論文の詳細を見る
We calculate the time dependent line and recombination spectrum of non-equilibrium plasma heated by strong radiation as a test model of X-ray line emission of GRB afterglows. Our calculation shows that the non-equilibrium effect of the plasma is complex and important in the time evolution of the spectrum. The origin of these lines is puzzling us, but it is essential to understand the nature of GRBs and their circumstellar matter.
- 理論物理学刊行会の論文
- 2004-11-15
著者
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Takabe Hideaki
Institute Of Laser Engineering Osaka University
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Takabe H
Osaka Univ. Osaka Jpn
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Takabe Hideaki
Institute Of Laser Energetics And Graduate School Of Science Osaka University
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Yamada Shoichi
Department Of Physics School Of Science The University Of Tokyo
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Yamada Shoichi
Department Of Physics Waseda University
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SUGIYAMA Shinya
Institute of Laser Engineering, Osaka University
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Sugiyama Shinya
Institute Of Laser Engineering Osaka University
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Takabe Hideaki
Institute For Laser Engineering Osaka University
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