Q: What determines the density spectrum of flows?
Q: What is the effect of the central star cluster?
Q: Do we need revised accretion disk models?
Q: Why are most/all flows dust-less?
Q: What happens at higher AGN luminosities?
Q: What happens in other accreting systems?
Mass Loss from AGN                      Doron Chelouche (IAS)
Text Box: Only Q’s
Only Q’s
Thank Q