Differential rotation is a key component of the Omega-effect, which
regenerates the large-scale toroidal magnetic fields during a dynamo
cycle, however, dynamos in different types of stars work in different
ways. In this talk, I aim to give an overview of how surface
differential rotation manifest on different types of stars (K dwarfs,
solar analogues, giant RS CVns, single giants, first lithium-dredge up,
etc) showcasing results on the topic from the last several
years, along with some implications of these results. Relations between
astrophysical parameters and differential rotation are also discussed.