Image Details
Caption: Figure 6.
KOREL output for two configurations: three disentangled components (top), line-strength of Star B vs phase of eclipsing pair (middle left), RV for star B (middle right), and RV for components in contact pair (bottom panels). Size of data points is proportional to S/N of input spectra.
© 2026. The Author(s). Published by the American Astronomical Society.