My talk will focus two different aspects of the same phenomenon: AGNs and their affect on galaxy evolution. We know from both observations and semi-analytic models that these processes must somehow be linked. However, how and when these links were forged is still some matter of debate. The first half of my talk will explore what insights into this relationship can be garnered from observations of AGNs at infrared wavelengths. Second, I will discuss some recent results which show that a significant fraction of all luminous AGNs have kinematically complex narrow line regions and place this in the context of feedback-inducing outflows.