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    請使用永久網址來引用或連結此文件: https://ir.lib.ncu.edu.tw/handle/987654321/101895


    題名: Period-Luminosity relations derived from the OGLE-III first-overtone mode Cepheids in the Magellanic Clouds
    作者: 饒兆聰;Bhardwaj, Anupam;Ngeow, Chow-Choong;Kanbur, Shashi M.;Singh, Harinder P.
    貢獻者: 理學院天文研究所
    關鍵詞: Breaking;Catalogues;Cepheid variables;Comparative analysis;Infrared;Luminosity;Magellanic clouds;Nonlinearity;Slopes;Star & galaxy formation;Statistical tests
    日期: 2016-03-17
    上傳時間: 2026-04-21 14:50:30 (UTC+8)
    出版者: Oxford University Press;London: Oxford University Press
    摘要: 摘要: We present multiband Period–Luminosity (PL) relations for first-overtone mode Cepheids in the Small Magellanic Cloud (SMC). We derive optical band PL relations and the Wesenheit function using VI mean magnitudes from the Optical Gravitational Lensing Experiment (OGLE-III) survey. We cross-match OGLE-III first-overtone mode Cepheids to the 2MASS and SAGE-SMC catalogues to derive PL relations at near-infrared (JHK s ) and mid-infrared (3.6 and 4.5 μm) wavelengths. We test for possible non-linearities in these PL relations using robust statistical tests and find a significant break only in the optical band PL relations at 2.5 d for first-overtone mode Cepheids. We do not find statistical evidence for a non-linearity in these PL relations at 1 d. The multiband PL relations for fundamental-mode Cepheids in the SMC also exhibit a break at 2.5 d. We suggest that the period break around 2.5 d is related to sharp changes in the light-curve parameters for SMC Cepheids. We also derive new optical and mid-infrared band PL relations for first-overtone mode Cepheids in the Large Magellanic Cloud (LMC). We compare multiband PL relations for first-overtone mode Cepheids in the Magellanic Clouds and find a significant difference in the slope of the V-band PL relations but not for I-band PL relations. The slope of PL relations are found to be consistent in most of the infrared bands. A relative distance modulus of Δμ = 0.49 ± 0.02 mag between the two clouds is estimated using multiband PL relations for the first-overtone mode Cepheids in the SMC and LMC.
    出版者: London: Oxford University Press
    出版日期: 2016-06-01
    出處: Monthly notices of the Royal Astronomical Society, 2016-06, Vol.458 (4), p.3705-3719
    資源來源: Alma/SFX Local Collection
    版權: 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society 2016
    版權: Copyright Oxford University Press, UK Jun 1, 2016
    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/stw579
    顯示於類別:[天文研究所] 期刊論文

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