Figure 9 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 9.

System configuration at the primary (left) and the secondary eclipse (right). The Cepheid center is marked by a blue ×, its minimum radius by a solid line and the range of radius change by a blue transparent color. The companion center is marked by a red + and the radius by the solid line. In both cases the width of the solid line represents the ±1σ radius error. The distances between the stars are about 650 R_⊙ and 725 R_⊙ at the primary and secondary eclipse, respectively.

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