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Abstract
Completing the massive star population: Striking into the field
Sally Oey (University of Michigan)
As a population, field massive stars are relatively enigmatic. With this contribution, I attempt to
illuminate this sector of the high-mass stellar population, which comprises 20 - 25% of the massive
stars in star-forming galaxies. "Field" massive stars appear to originate both in situ and as runaways
from clusters, and include not only OB stars, but also WR, Oe, and Be stars. I will review what is
known about the properties of massive field stars from studies in the Magellanic Clouds and the
Galaxy, addressing origins and properties like IMF, binarity, and rotation velocities. Comparison
between the field and cluster populations can then be used to probe star formation theory,
cluster evolution, and stellar evolution, while field star HII regions provide important constraints
on stellar atmosphere models.
(to be confirmed by the SOC)