Abstract:
Outflows serve as a crucial feedback mechanism in quasars, playing a significant
role in understanding the co-evolution processes between quasars and their host galaxies.
This paper collects and organizes literature on the research of velocity shifts in outflow ab#2;sorption lines, compares and analyzes the identification methods, challenges, and generation
mechanisms of such velocity shifts, and discusses potential future research directions. While
current empirical cases of absorption line velocity shifts are limited and their underlying
physical mechanisms remain unclear, the growth of quasar survey data and advancements in
data processing techniques are expected to lead to breakthroughs in this field, such progress
will not only deepen our understanding of quasar outflows, but also offer new perspectives
for galaxy evolution studies.