Supernovae and their associated binary disruptions can eject companion stars outward, contributing significantly to the observed population of runaway stars in the galaxy.
Evidence for · 2
Runaway OB Stars in the Small Magellanic Cloud. III. Updated Kinematics and Insights into Dynamical versus Supernova Ejections
2024 · cited by 16
Discusses the binary supernova scenario and how it ejects companion stars into the stellar field as runaways.
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Stellar ejection velocities from the binary supernova scenario: A comparison across population synthesis codes
2025 · cited by 4
Examines stellar ejection velocities from disrupted binary systems during supernovae, showing that companion stars are released with velocities related to their pre-supernova orbital motion.