  For the occasion of the official retirement of Henny Lamers, a meeting was
held to celebrate Henny's contribution to mass loss from stars and stellar
clusters. Stellar mass loss is crucial for understanding the life and death of
massive stars, as well as their environments. Henny has made important
contributions to many aspects of our understanding of hot-star winds. Here, the
most dominant aspects of the stellar part of the meeting: (i) O star wind
clumping, (ii) mass loss near the Eddington limit, and (iii) and the driving of
Wolf-Rayet winds, are highlighted.
