摘要: Centaurus A, the cosmic ray accelerator a few Mpc away from us, is possibly one of nearest sources extremely high energy rays. We investigate whether gamma data currently available A in GeV–TeV band can be explained with only proton–proton interactions. show that for single power law proton spectrum, mechanisms γ-ray production other than interactions are needed inside this radio-galaxy to explain flux observed by EGRET, upper limits HESS/CANGAROO-III and correlated energetic events Pierre Auger experiment. In future, better data, simultaneous observation detectors, it will possible carry out such studies on different more detail.