Mass and p-factor of the Type II Cepheid OGLE-LMC-T2CEP-098 in a Binary System
Authors: Bogumił Pilecki, Wolfgang Gieren, Radosław Smolec, Grzegorz Pietrzyński, Ian B. Thompson, Richard I. Anderson, Giuseppe Bono, Igor Soszyński, Pierre Kervella, Nicolas Nardetto, Mónica Taormina, Kazimierz Stȩpień, and Piotr Wielgórski
2017 The Astrophysical Journal842110.
Provider: AAS Journals
Caption: Figure 5.
I-band orbital light curve of the system, freed from the pulsations of the Cepheid. Both eclipses are well covered. The large difference in eclipse depths indicates a large difference in the temperatures of the component stars.