M. S. Oey

Professor

University of Michigan

United States

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About

Professor M. S. Oey is a faculty member at the University of Michigan, USA. His research focuses on the properties and dynamics of massive stars, stellar feedback mechanisms, and the interstellar medium, as demonstrated in his recent publications. He explores topics such as binary star systems in various environments and the impact of stellar activities on the escape of Lyman continuum radiation.

Articles (22)

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2025

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2020

Collaborators (5)

Göran Östlin

Stockholm University

SWEDEN

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John D Monnier

University of Michigan

UNITED STATES

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Yongjung Kim

Assistant Professor

Sejong University

SOUTH KOREA

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Edmund Hodges-Kluck

University of Michigan

UNITED STATES

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Milena Ratajczak

University of Warsaw

POLAND

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M. S. Oey

Research Interests

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About

Articles (22)

New Field OB and OBe Binaries of the SMC Wing: Observational Properties and Population Modeling

The Close Binary Properties of Massive Stars across Different Environments within the LMC

The Low-redshift Lyman Continuum Survey: The Roles of Stellar Feedback and Interstellar Medium Geometry in LyC Escape

The Effect of Radiation and Supernovae Feedback on LyC Escape in Local Star-forming Galaxies

Haro 11: The Spatially Resolved Lyman Continuum Sources

Runaway OB Stars in the Small Magellanic Cloud. III. Updated Kinematics and Insights into Dynamical versus Supernova Ejections

Kinematic Insights into Luminous Blue Variables and B[e] Supergiants

Strong Variability in AzV 493, an Extreme Oe-type Star in the SMC

Delayed Massive-star Mechanical Feedback at Low Metallicity

HST FUV Spectroscopy of Super Star Cluster A in the Green Pea Analog Mrk 71: Revealing the Presence of Very Massive Stars

Nebular C iv λ1550 Imaging of the Metal-poor Starburst Mrk 71: Direct Evidence of Catastrophic Cooling

Catastrophic Cooling in Superwinds. III. Nonequilibrium Photoionization

Classical OBe Stars as Post-supernova Runaways: Confirming Binary Origins

Massive-Star Feedback at Low Metallicity

Dynamical vs Supernova Acceleration of OB Stars in the Small Magellanic Cloud

Limits to Ionization-parameter Mapping as a Diagnostic of Hii Region Optical Depth

Catastrophic Cooling in Superwinds. II. Exploring the Parameter Space

Emission-line Wings Driven by Lyman Continuum in the Green Pea Analog Mrk 71

Numerical Modeling of Galactic Superwinds with Time-evolving Stellar Feedback

The Source of Leaking Ionizing Photons from Haro11: Clues from HST/COS Spectroscopy of Knots A, B, and C*

Conditions for Superwind Classes of Super Star Clusters

Spatially Resolved C iii] λ1909 Emission in Haro 11

Collaborators (5)

Göran Östlin

John D Monnier

Yongjung Kim

Edmund Hodges-Kluck

Milena Ratajczak

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