Young stellar population in the Lupus 3 molecular cloud

碩士 === 國立中央大學 === 天文研究所 === 94 === 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 Sch...

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Main Authors: Fong-Yi Huang, 黃峰毅
Other Authors: Wen-Ping Chen
Format: Others
Language:en_US
Published: 2006
Online Access:http://ndltd.ncl.edu.tw/handle/r3xg9d
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spelling ndltd-TW-094NCU051990062019-05-15T20:21:53Z http://ndltd.ncl.edu.tw/handle/r3xg9d Young stellar population in the Lupus 3 molecular cloud 豺狼三分子雲中的年輕星球 Fong-Yi Huang 黃峰毅 碩士 國立中央大學 天文研究所 94 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. Wen-Ping Chen 陳文屏 2006 學位論文 ; thesis 18 en_US
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description 碩士 === 國立中央大學 === 天文研究所 === 94 === 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.
author2 Wen-Ping Chen
author_facet Wen-Ping Chen
Fong-Yi Huang
黃峰毅
author Fong-Yi Huang
黃峰毅
spellingShingle Fong-Yi Huang
黃峰毅
Young stellar population in the Lupus 3 molecular cloud
author_sort Fong-Yi Huang
title Young stellar population in the Lupus 3 molecular cloud
title_short Young stellar population in the Lupus 3 molecular cloud
title_full Young stellar population in the Lupus 3 molecular cloud
title_fullStr Young stellar population in the Lupus 3 molecular cloud
title_full_unstemmed Young stellar population in the Lupus 3 molecular cloud
title_sort young stellar population in the lupus 3 molecular cloud
publishDate 2006
url http://ndltd.ncl.edu.tw/handle/r3xg9d
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