Pulsars, initially detected as radio sources, also emit in visible light, X-rays, and gamma rays. Newly formed neutron stars have temperatures between 10^{11} to 10^{12} kelvin, but this drops to around 10^{6} K within a few years due to energy loss from neutrinos. At this lower temperature, neutron stars primarily emit X-rays, while their rotational beams are observed in the radio spectrum. In visible light, neutron stars emit energy uniformly across the spectrum, appearing white. The discussion highlights the complexity of neutron star emissions and their varying wavelengths.