English  |  正體中文  |  简体中文  |  全文筆數/總筆數 : 94274/94274 (100%)
造訪人次 : 82857754      線上人數 : 1793
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: https://ir.lib.ncu.edu.tw/handle/987654321/101904


    題名: LSQ13fn: A type II-Plateau supernova with a possibly low metallicity progenitor that breaks the standardised candle relation∗
    作者: 陳婷琬;Polshaw, J.;Kotak, R.;Dessart, L.;Fraser, M.;Gal-Yam, A.;Inserra, C.;Sim, S. A.;Smartt, S. J.;Sollerman, J.;Baltay, C.;Rabinowitz, D.;Benetti, S.;Botticella, M. T.;Campbell, H.;Chen, T.-W.;Galbany, L.;McKinnon, R.;Nicholl, M.;Smith, K. W.;Sullivan, M.;Takáts, K.;Valenti, S.;Young, D. R.
    貢獻者: 理學院天文研究所
    關鍵詞: Astrophysics;Breaking;Candles;Imaging;Massive stars;Metallicity;Physics;Progenitors (astrophysics);Spectral emission;supernovae: general;supernovae: individual: LSQ13fn;Supernovas
    日期: 2016-04-01
    上傳時間: 2026-04-21 14:50:42 (UTC+8)
    出版者: EDP Sciences
    摘要: 摘要: We present optical imaging and spectroscopy of supernova (SN) LSQ13fn, a type II supernova with several hitherto-unseen properties. Although it initially showed strong symmetric spectral emission features attributable to He ii, N iii, and C iii, reminiscent of some interacting SNe, it transitioned into an object that would fall more naturally under a type II-Plateau (IIP) classification. However, its spectral evolution revealed several unusual properties: metal lines appeared later than expected, were weak, and some species were conspicuous by their absence. Furthermore, the line velocities were found to be lower than expected given the plateau brightness, breaking the SN IIP standardised candle method for distance estimates. We found that, in combination with a short phase of early-time ejecta-circumstellar material interaction, metal-poor ejecta, and a large progenitor radius could reasonably account for the observed behaviour. Comparisons with synthetic model spectra of SNe IIP of a given progenitor mass would imply a progenitor star metallicity as low as 0.1 Z⊙. LSQ13fn highlights the diversity of SNe II and the many competing physical effects that come into play towards the final stages of massive star evolution immediately preceding core-collapse.
    出版者: EDP Sciences
    出版日期: 2016-04-01
    出處: Astronomy and astrophysics (Berlin), 2016-04, Vol.588, p.A1
    資源來源: EDP Sciences
    版權: licence_http://creativecommons.org/publicdomain/zero
    識別號: ISSN: 0004-6361
    識別號: ISSN: 1432-0746
    識別號: EISSN: 1432-0746
    識別號: DOI: 10.1051/0004-6361/201527682
    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.html0KbHTML23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