M
M. S. Oey
Researcher at University of Michigan
Publications - 240
Citations - 13947
M. S. Oey is an academic researcher from University of Michigan. The author has contributed to research in topics: Galaxy & Stars. The author has an hindex of 57, co-authored 227 publications receiving 13086 citations. Previous affiliations of M. S. Oey include Steward Health Care System & University of Cambridge.
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An introduction to the chandra carina complex project
Leisa K. Townsley,Patrick S. Broos,Michael F. Corcoran,Michael F. Corcoran,Eric D. Feigelson,Marc Gagné,Thierry Montmerle,M. S. Oey,Nathan Smith,Gordon P. Garmire,Konstantin V. Getman,Matthew S. Povich,Nancy Remage Evans,Yaël Nazé,E. R. Parkin,E. R. Parkin,Thomas Preibisch,Junfeng Wang,Scott J. Wolk,You-Hua Chu,David H. Cohen,Robert A. Gruendl,Kenji Hamaguchi,Kenji Hamaguchi,Robert R. King,Mordecai-Mark Mac Low,Mark J. McCaughrean,Mark J. McCaughrean,Anthony F. J. Moffat,Lidia M. Oskinova,Julian M. Pittard,Keivan G. Stassun,Keivan G. Stassun,Asif ud-Doula,Nolan R. Walborn,Wayne L. Waldron,Ed Churchwell,Joy S. Nichols,Stanley P. Owocki,Norbert S. Schulz +39 more
TL;DR: In this paper, the authors have mapped the Carina star-forming complex in X-rays, using archival Chandra data and a mosaic of 20 new 60 ks pointings using the Chandra X-ray Observatory's Advanced CCD Imaging Spectrometer.
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A New Look at Simple Inhomogeneous Chemical Evolution
TL;DR: In this paper, a one-zone, closed-box model for inhomogeneous chemical evolution is proposed as an alternative reference to the Simple model in the limit of no mixing.
Posted Content
The Local Group as an Astrophysical Laboratory for Massive Star Feedback
TL;DR: In this paper, the authors reviewed studies of radiative and mechanical feedback in the Local Group and found that feedback plays a fundamental role in energy cycles on scales ranging from individual stars to cosmic structure.
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The Sparsest Clusters With O Stars
TL;DR: In this paper, the authors examined the mass ratio of the second-most massive and most massive stars (m_max,2/m-max), finding that their observations all exist below the 20th percentile of simulated clusters, although some are in the lowest 5th percentile frequency.
The IMF of Field OB Stars in the Small Magellanic Cloud
TL;DR: The Runaways and Isolated O Type Star Spectroscopic Survey of the Small Magellanic Cloud (RIOTS4) as discussed by the authors surveys a spatially complete sample of >350 field OB stars in the SMC and will serve as a key probe of runaways, binaries, and the stellar IMF in the field massive star population.