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APSIDAL MOTION AND A LIGHT CURVE SOLUTION FOR 13 LMC ECCENTRIC ECLIPSING BINARIES

  • Authors: P. Zasche, M. Wolf, J. Vraštil, and L. Pilarčík

2015 The Astronomical Journal 150 183.

  • Provider: AAS Journals

Caption: Figure 2.

OC diagrams for the times of minimum of the analyzed systems. The continuous and dashed curves represent predictions for the primary and secondary eclipses, respectively. The individual primary and secondary minima are denoted by dots and open circles, respectively. Larger symbols correspond to the more precise measurements. The bottom plots represent the residuals after subtraction of the fit.

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