Erratum: Stellar properties and nuclear matter constraints [Phys. Rev. C 93, 025806 (2016)]

Figure 1

Neutron star mass-radius relation. The horizontal bands indicate the masses of PSR J1614-2230 [1] (orange line) and PSR J038 + 0432 [2] (blue line).

Figure 2

Squared sound velocity for nuclear matter in the $\beta$ equilibrium. The orange dashed line represents the limit $v_s^2=\frac{1}{3}$.