  The origin and acceleration mechanisms of energetic particles in the universe
remain enigmatic in contemporary astrophysics. Recent efforts have focused on
identifying Galactic sources capable of accelerating particles to 1 PeV, known
as PeVatrons, and also identifying sources contributing to the spectrum at
lower energies. The different morphology of galactic supernova remnants is
directly related to the type of stellar explosion and the existence of a
possible Compact Central Object (CCO), which possess intense
radiativegravitational fields on their surfaces. These CCOs, due to their
strong fields and interactions with surrounding magnetic clouds, are potential
candidates for cosmic ray production. Through observations of the compact X-ray
source 1E 1207.4-5209, located near the remnant G296.5+10.0, and using the
enhanced GALPROP code, we analyze the emission of gamma-ray emission resulting
from cosmic-ray acceleration and propagation. Additionally, we calculate the
contribution of this association to the overall observed Galactic cosmic-ray
flux, considering cosmic-ray propagation within the Galaxy, including energy
losses and particle interactions. Our findings suggest that this setup offers a
fertile environment for producing a wide range of cosmic-ray energies at low
energy within the Galaxy.
