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Research on massive stars is undergoing a period of rapid progress,
with long-held convictions being shown to be incomplete. While
these stars are relatively few in number, they are the main driver
of chemical and dynamical evolution in galaxies through their
stellar winds and explosive deaths in core-collapse supernovae.
Furthermore the impact of massive stars is widely recognized in
many areas, as they are often used as tools to interpret the
conditions and processes arising in different environments. In
parallel, the development of new instrumentation, analysis
techniques and dedicated surveys across all possible wavelengths
have delivered large amounts of exquisite new data. These data are
now providing a harsh test for the current state-of-the-art
theoretical calculations of massive star birth, evolution and
death. IAU Symposium 329 covers these topics and is therefore an
invaluable resource for researchers in the field of massive stars
and their evolution.
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