| 研究生: |
姜博識 Po-Shih Chiang |
|---|---|
| 論文名稱: |
薔薇星雲中的X射線源 Stellar X-ray Sources in the Rosette Nebula |
| 指導教授: |
陳文屏
Wen-Ping Chen |
| 口試委員: | |
| 學位類別: |
碩士 Master |
| 系所名稱: |
理學院 - 天文研究所 Graduate Institute of Astronomy |
| 畢業學年度: | 91 |
| 語文別: | 英文 |
| 論文頁數: | 46 |
| 中文關鍵詞: | 年輕星球 |
| 外文關鍵詞: | X-ray, Young Stars |
| 相關次數: | 點閱:10 下載:0 |
| 分享至: |
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我們使用X-ray與光學觀測找尋薔薇星雲中的恆星X射線源。從ROSAT的網路資料庫中,我們找出了47個X射線源。利用光學影像、光譜、與光度資料,我們定出這些源的光學特性,並決定它們是否為薔薇星雲的成員星。最後,我們一共發現5個金牛座T型星與兩個赫比格AeBe星。並發現一個O型星可能有鋰吸收線,這暗示可能有低質量的年輕伴星。
We have used X-ray and optical observations to find the stellar X-ray sources in the
Rosette Nebula star-forming region. From $ROSAT$ archival data, we totally found 47 point
X-ray sources. We invetigate the optical properties of the X-ray sources by optical images,
photometry, and sprctroscopy, which allow us to distinguish among member stars in the region
from field stars. Five T Tauri stars and 2 Herbig Ae/Be stars have been identified by this
study. One O type star has been detected to have a weak 6707A Li absorption line,
indicating a possible young low-mass compaion.
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