English  |  正體中文  |  简体中文  |  全文筆數/總筆數 : 78937/78937 (100%)
造訪人次 : 39826021      線上人數 : 1285
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU 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://ir.lib.ncu.edu.tw/handle/987654321/50944


    題名: Whole Earth Telescope observations of the subdwarf B star KPD 1930+2752: a rich, short-period pulsator in a close binary
    作者: Reed,MD;Harms,SL;Poindexter,S;Zhou,AY;Eggen,JR;Morris,MA;Quint,AC;McDaniel,S;Baran,A;Dolez,N;Kawaler,SD;Kurtz,DW;Moskalik,P;Riddle,R;Zola,S;Ostensen,RH;Solheim,JE;Kepler,SO;Costa,AFM;Provencal,JL;Mullally,F;Winget,DW;Vuckovic,M;Crowe,R;Terry,D;Avila,R;Berkey,B;Stewart,S;Bodnarik,J;Bolton,D;Binder,PM;Sekiguchi,K;Sullivan,DJ;Kim,SL;Chen,WP;Chen,CW;Lin,HC;Jian,XJ;Wu,H;Gou,JP;Liu,Z;Leibowitz,E;Lipkin,Y;Akan,C;Cakirli,O;Janulis,R;Pretorius,R;Ogloza,W;Stachowski,G;Paparo,M;Szabo,R;Csubry,Z;Zsuffa,D;Silvotti,R;Marinoni,S;Bruni,I;Vauclair,G;Chevreton,M;Matthews,JM;Cameron,C;Pablo,H
    貢獻者: 天文研究所
    日期: 2011
    上傳時間: 2012-03-27 18:13:23 (UTC+8)
    出版者: 國立中央大學
    摘要: KPD 1930+2752 is a short-period pulsating subdwarf B (sdB) star. It is also an ellipsoidal variable with a known binary period of 2.3 h. The companion is most likely a white dwarf and the total mass of the system is close to the Chandresekhar limit. In this paper, we report the results of Whole Earth Telescope (WET) photometric observations during 2003 and a smaller multisite campaign of 2002. From 355 h of WET data, we detect 68 pulsation frequencies and suggest an additional 13 frequencies within a crowded and complex temporal spectrum between 3065 and 6343 mu Hz (periods between 326 and 157 s). We examine pulsation properties including phase and amplitude stability in an attempt to understand the nature of the pulsation mechanism. We examine a stochastic mechanism by comparing amplitude variations with simulated stochastic data. We also use the binary nature of KPD 1930+2752 for identifying pulsation modes via multiplet structure and a tidally induced pulsation geometry. Our results indicate a complicated pulsation structure that includes short-period (approximate to 16 h) amplitude variability, rotationally split modes, tidally induced modes and some pulsations which are geometrically limited on the sdB star.
    關聯: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
    顯示於類別:[天文研究所] 期刊論文

    文件中的檔案:

    檔案 描述 大小格式瀏覽次數
    index.html0KbHTML621檢視/開啟


    在NCUIR中所有的資料項目都受到原著作權保護.

    社群 sharing

    ::: Copyright National Central University. | 國立中央大學圖書館版權所有 | 收藏本站 | 設為首頁 | 最佳瀏覽畫面: 1024*768 | 建站日期:8-24-2009 :::
    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library IR team Copyright ©   - 隱私權政策聲明