English  |  正體中文  |  简体中文  |  全文筆數/總筆數 : 49378/84106 (59%)
造訪人次 : 7369261      線上人數 : 53
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library & TKU Library IR team.
搜尋範圍 查詢小技巧:
  • 您可在西文檢索詞彙前後加上"雙引號",以獲取較精準的檢索結果
  • 若欲以作者姓名搜尋,建議至進階搜尋限定作者欄位,可獲得較完整資料
  • 進階搜尋
    請使用永久網址來引用或連結此文件: http://tkuir.lib.tku.edu.tw:8080/dspace/handle/987654321/27851

    題名: Synthesis Imaging of Dense Molecular Gas in the N113 Hii Region of the Large Magellanic Cloud
    作者: Wong, Tony;Whiteoak, John B.;Ott, Juergen;秦一男;Chin, Yi-nan;Cunningham, Maria R.
    貢獻者: 淡江大學物理學系
    日期: 2006-09-20
    上傳時間: 2009-12-31 10:48:23 (UTC+8)
    出版者: American Astronomical Society
    摘要: We present aperture synthesis imaging of dense molecular gas in the Large Magellanic Cloud, taken with the prototype millimeter receivers of the Australia Telescope Compact Array (ATCA). Our observations of the N113 H II region reveal a condensation with a size of ~6'' (1.5 pc) FWHM, detected strongly in the 1-0 lines of HCO+, HCN, and HNC, and weakly in C2H. Comparison of the ATCA observations with single-dish maps from the Mopra Telescope and sensitive spectra from the Swedish-ESO Submillimetre Telescope indicates that the condensation is a massive clump of ~104 M☉ within a larger ~105 M☉ molecular cloud. The clump is centered adjacent to a compact, obscured H II region that is part of a linear structure of radio continuum sources extending across the molecular cloud. We suggest that the clump represents a possible site for triggered star formation. Examining the integrated line intensities as a function of interferometer baseline length, we find evidence for decreasing HCO+/HCN and HCN/HNC ratios on longer baselines. These trends are consistent with a significant component of the HCO+ emission arising in an extended clump envelope and a lower HCN/HNC abundance ratio in dense cores.
    關聯: Astrophysical Journal 649, pp.224-234
    DOI: 10.1086/504968
    顯示於類別:[物理學系暨研究所] 期刊論文


    檔案 描述 大小格式瀏覽次數
    0004-637X_649_1_224.pdf330KbAdobe PDF100檢視/開啟



    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library & TKU Library IR teams. Copyright ©   - 回饋