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The connection between AGB evolution of stellar populations and infrared vs.ultraviolet properties of the parent galaxies is reviewed relying on theupdated lookout provided by population-synthesis theory. In particular,planetary-nebula events and hot horizontal-branch evolution are assessed in aunitary view to outline a plain general picture of galaxy spectrophotometricevolution. This will include a brief discussion of relevant phenomena such asthe "UV upturn" in ellipticals and the stellar mass loss properties along thegalaxy morphological sequence.

Late stages of stellar evolution and their impact on spectrophotometric properties of galaxies