Are debris discs self-stirred?

@article{Kennedy2010AreDD,
  title={Are debris discs self-stirred?},
  author={Grant M. Kennedy and Mark C. Wyatt},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2010},
  volume={405},
  pages={1253-1270}
}
  • G. Kennedy, M. Wyatt
  • Published 18 February 2010
  • Geology, Physics
  • Monthly Notices of the Royal Astronomical Society
This paper aims to consider the evidence that debris disks are self-stirred by the formation of Pluto-size objects. A semi-analytical model for the dust produced during self-stirring is developed and applied to the statistics for A stars. We show that there is no significant statistical difference between fractional excesses of A-stars .50Myr old, and therefore focus on reproducing the broad trends, the “rise and fall” of the fraction of stars with excesses that the pre-stirred model of Wyatt… 

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