Neutron star
A supernovae occurs when a giant star collapses to the density of an atomic nucleus. At such a tremendous high densities, protons and electrons are fused together into neutrons. The neutrinos that are made in the iron core as protons are converted to neutrons. So after the explosion, the outer layers gets blow off in an often-spectacular display, leaving behind a sphere of tightly packed neutrons, a neutron star. It may roughly contain 10^57 neutrons with the mass between 1 and 3 solar masses. When the core of pre-supernovae star collapses into a neutron star, it's temperature can go up to trillions of degrees. At that particular point, star gives off gamma rays. Then it stars shrinking and cools. Initially the cooling is fast but as time passes it Starts cooling slowly. Because it has so little surface fir heat to radiate , it may have several thousands if degrees. Neutron stars even produce a significant amount of blackbody radiation . The