WEKO3
インデックスリンク
アイテム
Nonequilibrium Ionization States of Gamma-Ray Burst Environments
https://doi.org/10.24517/00010304
https://doi.org/10.24517/00010304c6a129a4-c1a1-45f2-a597-3eb1744b89cf
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
SC-PR-YONETOKU-D-23.pdf (149.6 kB)
|
.png)
|
| Item type | 学術雑誌論文 / Journal Article(1) | |||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| 公開日 | 2017-10-03 | |||||||||
| タイトル | ||||||||||
| タイトル | Nonequilibrium Ionization States of Gamma-Ray Burst Environments | |||||||||
| 言語 | ||||||||||
| 言語 | eng | |||||||||
| 資源タイプ | ||||||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||||||
| 資源タイプ | journal article | |||||||||
| ID登録 | ||||||||||
| ID登録 | 10.24517/00010304 | |||||||||
| ID登録タイプ | JaLC | |||||||||
| 著者 |
Yonetoku, Daisuke
× Yonetoku, Daisuke× Murakami, Toshio× Masai, Kuniaki× Yoshida, Atsumasa× Kawai, Nobuyuki× Namiki, Masaaki |
|||||||||
| 著者別表示 |
米德, 大輔
× 米德, 大輔
× 村上, 敏夫
|
|||||||||
| 提供者所属 | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | 金沢大学大学院自然科学研究科物理学 | |||||||||
| 書誌情報 |
The Astrophysical Journal 巻 557, 号 1, p. L23-L26, 発行日 2001-08-10 |
|||||||||
| ISSN | ||||||||||
| 収録物識別子タイプ | ISSN | |||||||||
| 収録物識別子 | 0004-637X | |||||||||
| NCID | ||||||||||
| 収録物識別子タイプ | NCID | |||||||||
| 収録物識別子 | AA00553242 | |||||||||
| DOI | ||||||||||
| 関連タイプ | isIdenticalTo | |||||||||
| 識別子タイプ | DOI | |||||||||
| 関連識別子 | 10.1086/323142 | |||||||||
| 出版者 | ||||||||||
| 出版者 | American Astronomical Society | |||||||||
| 抄録 | ||||||||||
| 内容記述タイプ | Abstract | |||||||||
| 内容記述 | Iron spectral features are thought to be the best tracers of progenitors of gamma-ray bursts (GRBs). The detections of spectral features such as an iron line and/or the radiative recombination edge and continuum (RRC) were reported in four X-ray afterglows of GRBs. However, burst for burst, their properties were different from each other. For example, the Chandra observation of GRB 991216 detected a strong H-like iron line together with the RRC. With ASCA, on the other hand, Yoshida and coworkers detected only the strong RRC in GRB 970828. Since it is difficult to produce the strong RRC, we have to consider a special condition for the line-and/or RRC-forming regions. In this Letter, we point out the possibility of a "nonequilibrium ionization state" for the line-and RRC-forming regions. | |||||||||
| 著者版フラグ | ||||||||||
| 出版タイプ | VoR | |||||||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||||||
