Figure 8 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 8.

Correlation between the inclination and the sum of the star radii. The χ² values are coded with color (higher values are darker). Solid lines represent 1, 2, and 3σ levels for the two-parameter error estimation. The best model is marked with a cross.

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