Abstract
In this paper, we have derived Cepheid period-luminosity (P-L) relations for the Large Magellanic Cloud (LMC) fundamental mode Cepheids, based on the data released from OGLE-III. We have applied an extinction map to correct for the extinction of these Cepheids. In addition to the VIW-band P-L relations, we also include JHK and four Spitzer IRAC-band P-L relations, derived by matching the OGLE-III Cepheids to the Two Micron All Sky Survey and SAGE data sets, respectively. We also test the nonlinearity of the Cepheid P-L relations based on extinction-corrected data. Our results (again) show that the LMC P-L relations are nonlinear in VIJH bands and linear in KW and the four IRAC bands, respectively. © 2009. The American Astronomical Society. All rights reserved.
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CITATION STYLE
Ngeow, C. C., Kanbur, S. M., Neilson, H. R., Nanthakumar, A., & Buonaccorsi, J. (2009). Period-luminosity relations derived from the ogle-III fundamental mode cepheids. Astrophysical Journal, 693(1), 691–696. https://doi.org/10.1088/0004-637X/693/1/691
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