Figure 3 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 3.

Fourier decomposition amplitudes and phases of the I-band light curve of the Cepheid in the OGLE LMC562.05.9009 system. The symbols on the Y-axes of the different panels have their usual meaning, and the data for the LMC Cepheids (small dots) come from the OGLE Survey (Soszyński et al. 2008). The light of the stable companion was subtracted from the Cepheid light curve before the analysis. The location of the Cepheid on all panels clearly supports fundamental mode pulsation, in agreement with the radius of the Cepheid derived from our analysis (see the text).

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