抜粋
We calculate the time-dependent line and recombination spectrum of nonequilibrium plasma heated by the strong radiation as the test model of X-ray line emission of GRB afterglows. Our calculation shows that the non-equilibrium effect of plasma is complex and important to the time evolution of the spectrum. The origin of these lines puzzles us, but is essential to understand the nature of GRBs and their circumstellar matter.
| 元の言語 | English |
|---|---|
| ページ（範囲） | 323-326 |
| ページ数 | 4 |
| ジャーナル | Astrophysics and Space Science |
| 巻 | 298 |
| 発行部数 | 1-2 |
| DOI | |
| 出版物ステータス | Published - 2005 6 1 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
フィンガープリント X-ray line and recombination emission in the afterglow of GRB' の研究トピックを掘り下げます。これらはともに一意のフィンガープリントを構成します。
これを引用
Sugiyama, S., Yamada, S., & Takabe, H. (2005). X-ray line and recombination emission in the afterglow of GRB. Astrophysics and Space Science, 298(1-2), 323-326. https://doi.org/10.1007/s10509-005-3962-9