The IMF of Field OB Stars in the Small Magellanic Cloud
J. B. Lamb, M. S. Oey, A. S. Graus, and D. M. Segura-Cox
University of Michigan Department of Astronomy, 830 Dennison Bldg., Ann Arbor, MI 48109-1042, USA
The population of field OB stars are an important component of a galaxy's stellar content, representing 20-30% of the massive stars. To study this population, we have undertaken the Runaways and Isolated O Type Star Spectroscopic Survey of the SMC (RIOTS4). RIOTS4 surveys a spatially complete sample of >350 field OB stars in the Small Magellanic Cloud and will serve as a key probe of runaways, binaries, and the stellar IMF in the field massive star population. Here, we focus on the field IMF, which provides an empirical probe of the star-forming process and is a fundamental property of a stellar population. Together with photometry from the OGLE survey, RIOTS4 will yield a definitive stellar IMF for the SMC field massive star population. We present preliminary results that suggests the field IMF is much steeper, Gamma = 2.9, than the canonical stellar IMF of Gamma = 1.35. Despite the steep slope, we see no evidence of a stellar upper mass limit, up to our highest mass star of 65 solar masses.
Reference: Four Decades of Research on Massive Stars, eds. L. Drissen, C. Robert, and N. St-Louis, ASP Conference Series
Status: Conference proceedings