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@ARTICLE{Sterken:207267,
      author       = {Sterken, Veerle J. and Westphal, Andrew J. and Altobelli,
                      Nicolas and Grün, Eberhard and Hillier, Jon K. and
                      Postberg, Frank and Srama, Ralf and Allen, Carlton and
                      Anderson, David and Ansari, Asna and Bajt, Saša and
                      Bastien, Ron S. and Bassim, Nabil and Bechtel, Hans A. and
                      Borg, Janet and Brenker, Frank E. and Bridges, John and
                      Brownlee, Donald E. and Burchell, Mark and Burghammer,
                      Manfred and Butterworth, Anna L. and Changela, Hitesh and
                      Cloetens, Peter and Davis, Andrew M. and Doll, Ryan and
                      Floss, Christine and Flynn, George and Frank, David and
                      Gainsforth, Zack and Heck, Philipp R. and Hoppe, Peter and
                      Hudson, Bruce and Huth, Joachim and Hvide, Brit and
                      Kearsley, Anton and King, Ashley J. and Lai, Barry and
                      Leitner, Jan and Lemelle, Laurence and Leroux, Hugues and
                      Leonard, Ariel and Lettieri, Robert and Marchant, William
                      and Nittler, Larry R. and Ogliore, Ryan and Ong, Wei Ja and
                      Price, Mark C. and Sandford, S. A. and Tresseras, Juan-Angel
                      Sans and Schmitz, Sylvia and Schoonjans, Tom and Silversmit,
                      Geert and Simionovici, Alexandre and Solé, Vicente A. and
                      Stephan, Thomas and Stodolna, Julien and Stroud, Rhonda M.
                      and Sutton, Steven and Trieloff, Mario and Tsou, Peter and
                      Tsuchiyama, Akira and Tyliszczak, Tolek and Vekemans, Bart
                      and Vincze, Laszlo and Korff, Joshua Von and Wordsworth,
                      Naomi and Zevin, Daniel and Zolensky, Michael E.},
      title        = {{S}tardust {I}nterstellar {P}reliminary {E}xamination {X}:
                      {I}mpact {S}peeds and {D}irections of {I}nterstellar
                      {G}rains on the {S}tardust {D}ust {C}ollector},
      journal      = {Meteoritics $\&$ planetary science},
      volume       = {49},
      number       = {9},
      issn         = {1086-9379},
      address      = {Hoboken, NJ},
      publisher    = {Wiley-Blackwell},
      reportid     = {PUBDB-2015-01250},
      pages        = {1680 - 1697},
      year         = {2014},
      note         = {(c) The Meteoritical Society. Post referee full text in
                      progress.},
      abstract     = {On the basis of an interstellar dust model compatible with
                      Ulysses and Galileo observations, we calculate and predict
                      the trajectories of interstellar dust (ISD) in the solar
                      system and the distribution of the impact speeds,
                      directions, and flux of ISD particles on the Stardust
                      Interstellar Dust Collector during the two collection
                      periods of the mission. We find that the expected impact
                      velocities are generally low (<10 km $s^{−1}$) for
                      particles with the ratio of the solar radiation pressure
                      force to the solar gravitational force β > 1, and that some
                      of the particles will impact on the cometary side of the
                      collector. If we assume astronomical silicates for particle
                      material and a density of 2 g cm$^{−3}$, and use the
                      Ulysses measurements and the ISD trajectory simulations, we
                      conclude that the total number of (detectable) captured ISD
                      particles may be on the order of 50. In companion papers in
                      this volume, we report the discovery of three interstellar
                      dust candidates in the Stardust aerogel tiles. The impact
                      directions and speeds of these candidates are consistent
                      with those calculated from our ISD propagation model, within
                      the uncertainties of the model and of the observations.},
      cin          = {FS-ML / DOOR},
      ddc          = {520},
      cid          = {I:(DE-H253)FS-ML-20120731 / I:(DE-H253)HAS-User-20120731},
      pnm          = {FS In-house research / external facilities (POF2-544)},
      pid          = {G:(DE-H253)POF2-Other-Beam-20130405},
      experiment   = {EXP:(DE-MLZ)External-20140101},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000342912100010},
      doi          = {10.1111/maps.12219},
      url          = {https://bib-pubdb1.desy.de/record/207267},
}