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.
- 一般社団法人日本物理学会の論文
- 2004-11-15
著者
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Yamada Shoichi
Department Of Physics School Of Science The University Of Tokyo
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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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YAMADA Shoichi
Department of Physics, The University of Tokyo
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YAMADA Shoichi
Department of Science and Engineering, Waseda University
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YAMADA Shoichi
Division of Pure and Applied Physics, Graduate School of Science and Engineering, Waseda University
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Yamada Shoichi
Department of Chemistry, University of Tsukuba
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