抄録
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.
| 本文言語 | English |
|---|---|
| ページ（範囲） | 419-420 |
| ページ数 | 2 |
| ジャーナル | Progress of Theoretical Physics Supplement |
| 巻 | 155 |
| DOI | |
| 出版ステータス | Published - 2004 |
ASJC Scopus subject areas
- 物理学および天文学（その他）