Scientific Program Talks and Posters Pictures from the Meeting

Massive stars are extremely rare: for every 20Mo star in the Milky Way there are roughly a hundred thousand solar-type stars; for every 100 Mo star there should be over a million solar-type stars. In part this is due to their short lifetimes (a few million years) and the power-law nature of the initial mass function. Nevertheless, these rare objects exert a disproportional influence over their environments during their lifetimes. Through the actions of their strong stellar winds and eventual disruption as supernovae, they provide most of the mechanical input into the ISM. They also provide most of the UV ionizing radiation in galaxies, and power the far-IR luminosities through the heating of dust. And, massive stars serve as the primary source of carbon, nitrogen, and oxygen enrichment in the universe. They are also believed to be the source of the most energetic phenomenon yet found, emitting gamma-ray bursts as they collapse into blacko holes.

This workshop is aimed at honoring the scientific accomplishments of Peter S. Conti, who has also had a lifetime of influence over the field of massive star research. The workshop will consist of invited and contributed talks on current research plus posters, and will cover the following topics: