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.