Compact remnant supported by neutron-degeneracy pressure (and repulsive strong force); M ≈ 1.4–2 M_☉, R ≈ 10 km. Observed as pulsars.
Compact remnant supported by neutron-degeneracy pressure (and repulsive strong force); M ≈ 1.4–2 M_☉, R ≈ 10 km. Observed as pulsars.