An Analytic Technique for Constraining the Dynamical Origins of Multiple Star Systems Containing Merger Products
Nathan Leigh, Alison Sills

TL;DR
This paper introduces an analytic method to determine the dynamical formation scenarios of multiple star systems with merger products, using energy conservation to trace back their initial conditions and assess their origins.
Contribution
The authors develop a novel analytic technique to constrain the dynamical origins of multiple star systems with merger products, applicable to observed systems like blue stragglers.
Findings
Both S1082 and many blue straggler binaries in NGC 188 could have a dynamical origin.
Encounters involving triples may significantly contribute to blue straggler populations.
The method estimates encounter timescales based on initial orbital parameters.
Abstract
We present a technique to identify the most probable dynamical formation scenario for an observed binary or triple system containing one or more merger products or, alternatively, to rule out the possibility of a dynamical origin. Our method relies on an analytic prescription for energy conservation during stellar encounters. With this, observations of the multiple star system containing the merger product(s) can be used to work backwards in order to constrain the initial orbital energies of any single, binary or triple systems that went into the encounter. The initial semi-major axes of the orbits provide an estimate for the collisional cross section and therefore the time-scale for the encounter to occur in its host cluster. We have applied our analytic prescription to observed binary and triple systems containing blue stragglers, in particular the triple system S1082 in M67 and the…
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