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Galaxies form out of small fluctuations in a smoothly expanding Universe.However, the initial gravitational collapse phase is accompanied by theformation of supermassive black holes and clusters of massive stars. Blackholes and star clusters generate powerful outflows in the form of jets andsuperwinds that interact with still infalling gas, possibly regulating thegalaxy formation process, initiating new sites of star formation, and carryingchemically enriched gas to the intergalactic medium. Unfortunately, beyond thisqualitative description our detailed theoretical understanding is poor.  New results from 3D simulations of a GPS/CSS galaxy, with gravitationalpotentials included, shed some new light on the jet driven outflow process inparticular. New code capabilites to predict detailed X-ray spectra frommulti-dimensional time-dependent dynamics simulations of Galaxy Feedback, andwill be useful for future interpretation of X-ray and radio SEDs of forminggalaxies.Comment: 10 pages, 5 figures, Invited Conference Talk, The Spectral Energy  Distribution of Gas Rich Galaxies: Confronting Models with Data, Heidelberg,  Germany,October 4-8, 200

3D ISM-Shock Spectral Emission: X-ray models for Radio Galaxy SED Modeling