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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

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Figure

Figure 1. Photometric data collected for LMC562.05.9009. Upper panel:
Figure 4. I-band orbital light curve of the system determined from OGLE data, freed from the pulsations of the Cepheid
Figure 6. Pulsational radial velocity curve (black circles) and radius variation of the Cepheid over one pulsation cycle (solid line)
Figure 8. Correlation between the inclination and the sum of the star radii. The χ 2 values are coded with color (higher values are darker)
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