抜粋
In this paper, we present a study of the expanding HII region RCW 89 which is thought to be a part of the radio supernova remnant MSH 15-52 and its associated young 150 ms pulsar B1509-58. We had measured the proper motion of each of the plasma clouds in RCW 89, revealing that these plasma clouds have moved outwards from the SNR center. In order to resolve what is moving at a velocity of ∼5600km/s, we performed spectroscopic analysis of each of the plasma clouds using XMM-Newton and found that each plasma cloud has significantly different redshift. This result strongly suggests that the X-ray emission in RCW 89 comes from the fast expanding SN ejecta.
| 元の言語 | English |
|---|---|
| ホスト出版物のタイトル | 40 Years Of Pulsars |
| ホスト出版物のサブタイトル | Millisecond Pulsars, Magnetars and More |
| ページ | 219-221 |
| ページ数 | 3 |
| DOI | |
| 出版物ステータス | Published - 2008 3 20 |
| イベント | 40 Years Of Pulsars: Millisecond Pulsars, Magnetars and More - Montreal, QC, Canada 継続期間: 2007 8 12 → 2007 8 17 |
出版物シリーズ
| 名前 | AIP Conference Proceedings |
|---|---|
| 巻 | 983 |
| ISSN（印刷物） | 0094-243X |
| ISSN（電子版） | 1551-7616 |
Conference
| Conference | 40 Years Of Pulsars: Millisecond Pulsars, Magnetars and More |
|---|---|
| 国 | Canada |
| 市 | Montreal, QC |
| 期間 | 07/8/12 → 07/8/17 |
ASJC Scopus subject areas
- Physics and Astronomy(all)
フィンガープリント A study of rapid expanding H II region RCW 89' 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
Yatsu, Y., Kawai, N., Kataoka, J., & Brinkmann, W. (2008). A study of rapid expanding H II region RCW 89. ： 40 Years Of Pulsars: Millisecond Pulsars, Magnetars and More (pp. 219-221). (AIP Conference Proceedings; 巻数 983). https://doi.org/10.1063/1.2900147