1.3 1.4 1.5 1.6 10 12 14 16 R (km) 1.4 1.6 1.8 APR SLY4 BSR10 TM1 NL3 G$_{D}$=1.2G$_{S}$ G$_{V}$=0.1 G$_{D}$=1.2G$_{S}$ G$_{V}$=0.2 M (M O ) FIG. 5: (Color online) Plots for the mass-radius relationships for the equilibrium sequences of the non- rotating compact stars obtained using various EOSs as shown in Fig. 3. The solid circles and triangles divide the curves according to the composition of the hybrid stars as described in Fig. 4. 17