The Cepheid Period-Luminosity Relation in the Large Magellanic Cloud
A homogeneous set of ground-based BVRI observations of ∼600 Cepheids is presented to check the Cepheid period-luminosity zero point for the Large Magellanic Cloud (LMC). The sample of Cepheids is completely self-contained and has been reduced consistent
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
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