X-ray line and recombination emission in the afterglow of GRB

S. Sugiyama, S. Yamada, H. Takabe

研究成果: Article

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
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