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    Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/5994

    Title: 薔薇星雲中的X射線源;Stellar X-ray Sources in the Rosette Nebula
    Authors: 姜博識;Po-Shih Chiang
    Contributors: 天文研究所
    Keywords: 年輕星球;X-ray;Young Stars
    Date: 2002-09-30
    Issue Date: 2009-09-22 10:11:36 (UTC+8)
    Publisher: 國立中央大學圖書館
    Abstract: 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.
    Appears in Collections:[天文研究所] 博碩士論文

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