博碩士論文 93229003 完整後設資料紀錄

DC 欄位 語言
DC.contributor天文研究所zh_TW
DC.creator黃峰毅zh_TW
DC.creatorFong-Yi Huangen_US
dc.date.accessioned2006-7-14T07:39:07Z
dc.date.available2006-7-14T07:39:07Z
dc.date.issued2006
dc.identifier.urihttp://ir.lib.ncu.edu.tw:444/thesis/view_etd.asp?URN=93229003
dc.contributor.department天文研究所zh_TW
DC.description國立中央大學zh_TW
DC.descriptionNational Central Universityen_US
dc.description.abstract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。zh_TW
dc.description.abstractWe 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.en_US
DC.subject恆星形成zh_TW
DC.subjectstar formationen_US
DC.title豺狼三分子雲中的年輕星球zh_TW
dc.language.isozh-TWzh-TW
DC.titleYoung stellar population in the Lupus 3 molecular clouden_US
DC.type博碩士論文zh_TW
DC.typethesisen_US
DC.publisherNational Central Universityen_US

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