Fig. 2
Range of neutron-star masses and radii for the unified Brussels-Montreal EoSs (Goriely et al. 2010). The shaded area reflects the different degrees of stiffness of these EoSs: the lower limit corresponds to BSk19, the upper to BSk21. For comparison, we have indicated the measured mass of PSR J1614−2230 including estimated errors from Demorest et al. (2010).
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