Shadow cast and center of mass energy in a charged Gauss-Bonnet-AdS black hole

This work is devoted to the exploration of shadow cast and center mass energy in background a 4-dimensional charged Gauss-Bonnet AdS black hole. On investigating particle dynamics, we have examined BH's metric function. Whereas, with help null geodesics, pursue calculate celestial coordinates radius We made use hawking temperature study emission rate. Moreover, explored discussed its characteristics under influence spacetime parameters. For better understanding, graphically represent all our main findings. The acquired result shows that both charge ($l$) decrease radius, while coupling parameter $\alpha$ increases spacetime. other hand, $Q$ diminishing asymptotically flat Finally, investigate rate $\alpha$.