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研究生: 黃峰毅
Fong-Yi Huang
論文名稱: 豺狼三分子雲中的年輕星球
Young stellar population in the Lupus 3 molecular cloud
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: 94
語文別: 英文
論文頁數: 18
中文關鍵詞: 恆星形成
外文關鍵詞: star formation
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  • 我們利用UKST的Hα巡天計劃之影像資料庫,來尋找具有發射線的星球。研究的目標是豺狼座恆星形成區,為距離地球最近的恆星形成區之一。我們分析了一個視野大小為30 x 30角分的影像,此影像的中心為豺狼3分子雲中的兩顆赫比Ae星,找出了46顆具Hα發射線之傳統金牛座T型星候選者,其中22顆為新發現的。這22顆中的其中7顆星的2MASS近紅外顏色與傳統金牛座T型星相符。一旦光譜觀測能確定這些候選星為新發現的傳統金牛座T型星,它們將增加該區域的年輕恆星數量,並提供研究該分子雲恆星形成歷史的基本樣本。


    We report a pilot study to identify emission-line stars by use of the image database of the hydrogen-alpha survey by the United Kingdom Schmidt Telescope. The Lupus dark clouds are among the nearest star-forming regions. We analyzed a 30’ x 30’ field of the UK Schmidt Hα images centered around the 2 Herbig Ae stars of the Lupus 3 cloud. A list of 46 candidate T Tauri stars have been identified, among which 22 are new identifications. Seven out of these 22 Hα stars have 2MASS infrared colors consistent with being classical T Tauri stars. Once the candidates are spectroscopically confirmed, these stars will add to the young stellar sample in the region to study the star formation process in the molecular cloud.

    1. Introduction 1 1.1 The Lupus 3 molecular cloud 2 1.2 The UKST Hα survey 3 1.3 2MASS 5 2. Data reduction and analysis 6 2.1 UKST images 6 2.2 Spectroscopic data 9 3. Results and discussion 10 3.1 CTTS candidates by Hα images and IR colors 10 3.2 Spectra of CTTS candidates 14 3.3 Discussion 15 3.4 Conclusion 17 Bibliography 18

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