Fig. 29
Masses vs. radii of J150822 and J160156 components (squares) compared with 32 components of low-mass detached binaries (diamonds) from Torres et al. (2010) and 20 components of short-period contact binaries (triangles) from Stepień & Gazeas (2012). Also plotted are theoretical isochrones derived from Dartmouth models (Dotter et al. 2008) for solar metallicity, with ages of 0.25, 1, 5, and 10 Gyr, respectively (dotted lines, ascending).
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