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    Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/69903


    Title: 吸積雙星中致密天體與吸積盤特性之進一步研究;Further Studies of Compact Objects and Accretion Disks in Accreting Binaries
    Authors: 周翊
    Contributors: 天文研究所
    Keywords: X 光雙星;激變變星;吸積;吸積盤;白矮星;中子星;黑洞;超軌道光變;_x000d_ 希爾伯特-黃轉換;超駝峰光變;脈衝星;毫秒脈衝星;吸積型態之毫秒脈衝星;準週_x000d_ 期震盪;X-ray binary;cataclysmic variable;accretion;accretion disk;white dwarf;_x000d_ neutron star;black hole;superorbital modulation;Hilbert-Huang transfer;superhump_x000d_ variation;pulsar;millisecond pulsar;物理;太空科技
    Date: 2016-03-29
    Issue Date: 2016-03-30 09:51:31 (UTC+8)
    Publisher: 科技部
    Abstract: 我們將在本計畫中持續針對吸積雙星中的致密天體與吸積盤做深入的研究。吸積雙 星,包括了X 光雙星與激變變星,在是天文中對致密天體與吸積現象研究之主要天體之 一。在本計畫中,我們持續將先進的時序分析法—希爾伯特-黃轉換應用在分析超軌道 光變外,也將應用到X 光雙星中的準週期震盪的研究上,準週期震盪之不穩定性可能是 由於震盪周期或振幅隨時間而變,而希爾伯特-黃轉換能解析出瞬時之光變週期與振 幅,成為分析上述二種現象之有力工具。另一方面,結合帕洛瑪瞬變工廠之可見光資料 與從X 光望遠鏡的監測資料,我們可以取得同步;We propose to continue our studies on the properties of the compact objects and the accretion disks in accreting binaries. The accreting binaries with compact objects as accretors, including X-ray binaries and cataclysmic variables, are important astrophy;研究期間:10408~10507
    Relation: 財團法人國家實驗研究院科技政策研究與資訊中心
    Appears in Collections:[天文研究所] 研究計畫

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