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The runaway process is only halted when binary stars form at
the centre through 3-body encounters.
This may happen e.g. when a single star passes two others,
which may or may not be already a physical pair.
If the passage is close enough, it interacts with the
individual components seperately.
These interactions can be very complex in general, resulting
in the formation of a temporary triple-star system,
the disruption of the former binary, or the exchange of partners.
The figure shows a typical interaction between the stars:
a single star (green) comes in from the left and meets
a binary from the right (red + white).
After the dissociation of the binary, a chaotic
behaviour sets in wherein different other orbits are formed
and disrupted (red + green), and in the end, a harder binary
than before (more tightly bound) is created, while one spare
star escapes to infinity.
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Interaction of a binary with a single star
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