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@ARTICLE{Bhandare:865455,
      author       = {Bhandare, Asmita and Pfalzner, Susanne},
      title        = {{DESTINY}: {D}atabase for the {E}ffects of {ST}ellar
                      encounters on d{I}sks and pla{N}etary s{Y}stems},
      journal      = {Computational Astrophysics and Cosmology},
      volume       = {6},
      number       = {1},
      issn         = {2197-7909},
      address      = {New York, NY [u.a.]},
      publisher    = {Springer international},
      reportid     = {FZJ-2019-04905},
      pages        = {3},
      year         = {2019},
      abstract     = {Most stars form as part of a stellar group. These young
                      stars are mostly surrounded by a disk from which potentially
                      a planetary system might form. Both, the disk and later on
                      the planetary system, may be affected by the cluster
                      environment due to close fly-bys. The here presented
                      database can be used to determine the gravitational effect
                      of such fly-bys on non-viscous disks and planetary systems.
                      The database contains data for fly-by scenarios spanning
                      mass ratios between the perturber and host star from 0.3 to
                      50.0, periastron distances from 30 au to 1000 au, orbital
                      inclination from 0∘ to 180∘ and angle of periastron of
                      0∘, 45∘ and 90∘. Thus covering a wide parameter space
                      relevant for fly-bys in stellar clusters. The data can
                      either be downloaded to perform one's own diagnostics like
                      for e.g. determining disk size, disk mass, etc. after
                      specific encounters, obtain parameter dependencies or the
                      different particle properties can be visualized
                      interactively. Currently the database is restricted to
                      fly-bys on parabolic orbits, but it will be extended to
                      hyperbolic orbits in the future. All of the data from this
                      extensive parameter study is now publicly available as
                      DESTINY.},
      cin          = {JSC},
      ddc          = {530},
      cid          = {I:(DE-Juel1)JSC-20090406},
      pnm          = {511 - Computational Science and Mathematical Methods
                      (POF3-511)},
      pid          = {G:(DE-HGF)POF3-511},
      typ          = {PUB:(DE-HGF)16},
      doi          = {10.1186/s40668-019-0030-3},
      url          = {https://juser.fz-juelich.de/record/865455},
}