Figure 2 from THE ARAUCARIA PROJECT: A STUDY OF THE CLASSICAL CEPHEID IN THE ECLIPSING BINARY SYSTEM OGLE LMC562.05.9009 IN THE LARGE MAGELLANIC CLOUD

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THE ARAUCARIA PROJECT: A STUDY OF THE CLASSICAL CEPHEID IN THE ECLIPSING BINARY SYSTEM OGLE LMC562.05.9009 IN THE LARGE MAGELLANIC CLOUD

Authors: Wolfgang Gieren, Bogumił Pilecki, Grzegorz Pietrzyński, Dariusz Graczyk, Andrzej Udalski, Igor Soszyński, Ian B. Thompson, Pier Giorgio Prada Moroni, Radosław Smolec, Piotr Konorski, Marek Górski, Paulina Karczmarek, Ksenia Suchomska, Mónica Taormina, Alexandre Gallenne, Jesper Storm, Giuseppe Bono, Márcio Catelan, Michał Szymański, Szymon Kozłowski , Paweł Pietrukowicz, Łukasz Wyrzykowski, Radosław Poleski, Jan Skowron, Dante Minniti, K. Ulaczyk, P. Mróz, M. Pawlak, and Nicolas Nardetto

2015 The Astrophysical Journal 815 28.

Provider: AAS Journals

Caption: Figure 2.

Out-of-eclipse pulsational light curves of the Cepheid in the LMC562.05.9009 system, freed from the companion light and folded with the ephemeris T_max (HJD) = 2454507.90 + 2.987846×E. The magnitudes in this figure have not been dereddened. The Y-axis span is always the same (0.85 mag)—one can see that the amplitude is smaller for the redder filters.

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