Probing Low-Luminosity Gamma-Ray Emission from SNR G296.5+10.0 and CCO 1E 1207.4-5209 with CTAO
This study models the transport of cosmic rays and the gamma-ray emission from SNR G296.5+10.0 and the associated CCO 1E 1207.4-5209, showing that the Cherenkov Telescope Array Observatory (CTAO) can detect the characteristic hadronic and leptonic emissions of this unique system to provide, for the first time, constraints on particle acceleration in environments of luminosity-weak CCO supernova remnants.