OGLE Cepheids have Lower Amplitudes in SMC than in LMC
Bohdan Paczynski, Bart Pindor
Abstract
We selected cepheids from the OGLE database for the Magellanic Clouds in the period range 101.1 < P < 101.4 days. There were 33 objects in the LMC and 35 in the SMC. We find that the median amplitude of cepheids in the LMC is 18% larger than in the SMC, a 4 sigma effect. This implies that the period - flux amplitude relation is not universal, and cannot be used to measure distances accurately.
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