The runaway binary Mel 34 was ejected from R136 52,000 years ago in a five-body encounter between the binary Mel 39 with an orbiting third star VFTS 590 and the binary Mel 34.
We can limit the available parameter space enormously by requirements that energy, and momentum (linear and angular) are conserved througout the interaction
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The origin of the most recently ejected OB runaway star from the R136 cluster
The runaway binary Mel 34 was ejected from R136 52,000 years ago in a five-body encounter between the binary Mel 39 with an orbiting third star VFTS 590 and the binary Mel 34.