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We present results from models of galactic winds driven by energy injected bynuclear starbursts. The total energy of the starburst is provided by youngcentral stellar clusters and parts of the galactic interstellar medium arepushed out as part of the galactic wind (in some cases the galactic windcontains an important part of the metals produced in the new generation ofstars). We have performed adiabatic and radiative 3D N-Body/Smooth ParticleHydrodynamics simulations of galactic winds using the GADGET-2 code. Thenumerical models cover a wide range of starburst (from $\sim10^2$ to $\sim10^7$M$_\odot$) and galactic gas masses (from $\sim6\times10^6$ to $\sim10^{11}$M$_\odot$). The concentrated central starburst regions are an efficient enginefor producing of the mass and metal loss in galaxies, and also for driving themetal redistribution in the galaxies.

Mass and metal ejection efficiency in disk galaxies driven by young stellar clusters of nuclear starburst