中大學術數位典藏-NCU Institutional Repository-提供博碩士論文、考古題、期刊論文、研究計畫等下載:Item 987654321/101301
English  |  正體中文  |  简体中文  |  Items with full text/Total items : 94201/94201 (100%)
Visitors : 81545584      Online Users : 3998
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library IR team.
Scope Tips:
  • please add "double quotation mark" for query phrases to get precise results
  • please goto advance search for comprehansive author search
  • Adv. Search
    HomeLoginUploadHelpAboutAdminister Goto mobile version


    Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/101301


    Title: Long-term X-ray variability of ultraluminous X-ray sources
    Authors: 周翊;Lin, Lupin Chun-Che;Hu, Chin-Ping;Kong, Albert K. H.;Yen, David Chien-Chang;Takata, Jumpei;Chou, Yi
    Contributors: 理學院天文研究所
    Keywords: Accretion disks;Binary stars;Dynamic tests;Galaxies;Milky Way;Modulation;Orbitals;Star & galaxy formation;X-ray astronomy;X-ray sources;X-rays
    Date: 2015-01-01
    Issue Date: 2026-04-21 14:29:49 (UTC+8)
    Publisher: Oxford University Press;London: Oxford University Press
    Abstract: 摘要: Long-term X-ray modulations on time-scales from tens to hundreds of days have been widely studied for X-ray binaries located in the Milky Way and the Magellanic Clouds. For other nearby galaxies, only the most luminous X-ray sources can be monitored with dedicated observations. We here present the first systematic study of long-term X-ray variability of four ultraluminous X-ray sources (ESO 243-49 HLX-1, Holmberg IX X-1, M81 X-6, and NGC 5408 X-1) monitored with Swift. By using various dynamic techniques to analyse their light curves, we find several interesting low-frequency quasi-periodicities. Although the periodic signals may not represent any stable orbital modulations, these detections reveal that such long-term regular patterns may be related to superorbital periods and structure of the accretion discs. In particular, we show that the outburst recurrence time of ESO 243-49 HLX-1 varies over time and suggest that it may not be the orbital period. Instead, it may be due to some kinds of precession, and the true binary period is expected to be much shorter.
    出版者: London: Oxford University Press
    出版日期: 2015-12-01
    出處: Monthly notices of the Royal Astronomical Society, 2015-12, Vol.454 (2), p.1644-1657
    資源來源: Alma/SFX Local Collection
    版權: 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society 2015
    版權: Copyright Oxford University Press, UK Dec 1, 2015
    識別號: ISSN: 0035-8711
    識別號: ISSN: 1365-8711
    識別號: ISSN: 1365-2966
    識別號: EISSN: 1365-2966
    識別號: DOI: 10.1093/mnras/stv2025
    Appears in Collections:[Graduate Institute of Astronomy] journal & Dissertation

    Files in This Item:

    File Description SizeFormat
    index.html0KbHTML23View/Open


    All items in NCUIR are protected by copyright, with all rights reserved.

    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