ESO Workshop, ESO Headquarters, Garching, Germany, 6–10 July, 2015
Mass loss from cool Asymptotic Giant Branch and Red Supergiant stars inputs large amounts of material to the ISM and is therefore an important process for understanding stellar lifecycles and galactic ecology. Significant advances in observations (e.g. VLTI, ALMA and other facilities), and theory, now provide an opportunity to revisit outstanding questions of late stellar evolution, such as the role of mass loss, magnetic fields and binarity. The aim of the meeting is to bring together observers and theorists from the low and high mass stellar communities with the goals of exploring the commonalities of evolved star mass loss.