Modeling stellar winds on the asymptotic giant branch accurately

I present the latest progress on our ongoing work with our state-of-the-art
models of stellar winds of asymptotic giant branch stars. I will both depict
features and assumptions of our model code T-800 and show some of the results
that set our work apart; because, results are in several a case drastically
different from earlier results. In particular, I focus on effects of
gas-to-dust drift and higher-than-before spatial resolution.