Where the Solar system meets the solar neighbourhood: patterns in the distribution of radiants of observed hyperbolic minor bodies

@article{Marcos2018WhereTS,
  title={Where the Solar system meets the solar neighbourhood: patterns in the distribution of radiants of observed hyperbolic minor bodies},
  author={Carlos de la Fuente Marcos and Ra{\'u}l de la Fuente Marcos and Sverre J. Aarseth},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2018},
  volume={476}
}
Observed hyperbolic minor bodies might have an interstellar origin, but they can be natives of the Solar system as well. Fly-bys with the known planets or the Sun may result in the hyperbolic ejection of an originally bound minor body; in addition, members of the Oort cloud could be forced to follow inbound hyperbolic paths as a result of secular perturbations induced by the Galactic disc or, less frequently, due to impulsive interactions with passing stars. These four processes must leave… 

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