2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/15260We carried out the Gaussian fitting to the profile of PSR B1237+25 and found that six components rather than five are necessary to make a good fit. In the central part, we found that the core emission is not filled pencil beam but is a small hollow cone. This implies that the impact angle could be $β<0.5^\circ$. The ``hollow core'' is in agreement with Inverse Compton Scattering model of radio pulsars.2 pages, no figures, LaTeXAstrophysicstext