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    Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/50799


    Title: THE MID-INFRARED PERIOD-LUMINOSITY RELATIONS FOR THE SMALL MAGELLANIC CLOUD CEPHEIDS DERIVED FROM SPITZER ARCHIVAL DATA
    Authors: Ngeow,CC;Kanbur,SM
    Contributors: 天文研究所
    Keywords: GRAVITATIONAL LENSING EXPERIMENT.;FUNDAMENTAL-MODE CEPHEIDS;AMPLITUDE-COLOR RELATIONS;OGLE-III CATALOG;CLASSICAL CEPHEIDS;HUBBLE CONSTANT;SPACE-TELESCOPE;DARK ENERGY;LEAVITT LAW;LMC DATA
    Date: 2010
    Issue Date: 2012-03-27 18:10:22 (UTC+8)
    Publisher: 國立中央大學
    Abstract: In this paper, we derive the Spitzer IRAC band period luminosity (P-L) relations for the Small Magellanic Cloud (SMC) Cepheids, by matching the Spitzer archival SAGE-SMC data with the OGLE-III SMC Cepheids. We find that the 3.6 mu m and 4.5 mu m band P L relations can be better described using two P-L relations with a break period at log(P) = 0.4: this is consistent with similar results at optical wavelengths for SMC P-L relations. The 5.8 mu m and 8.0 mu m band P-L relations do not extend to sufficiently short periods to enable a similar detection of a slope change at log(P) = 0.4. The slopes of the SMC P-L relations, for log(P) > 0.4, are consistent with their Large Magellanic Cloud counterparts that were derived from a similar data set. They are also in agreement with those obtained from a small sample of Galactic Cepheids with parallax measurements.
    Relation: ASTROPHYSICAL JOURNAL
    Appears in Collections:[Graduate Institute of Astronomy] journal & Dissertation

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