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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
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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.

    1. Introduction 1.1 The Rosette Nebula 1.2 Young Stellar Population 2. Data Reduction and Analysis 2.1 ROSAT X-ray Archival Data 2.2 Photometric Data and KPNO Optical Narrow-band Images 2.3 BAO Optical Spectra 3. Results and Discussion 3.1 X-ray Perproties 3.2 Optical Properties of the X-ray Sources 3.3 Individual SOurces 4. Conclusions Appdex A. Spectra of All Sources Appdex B. Finding Charts

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