Collisional Grooming Models of the Kuiper Belt Dust Cloud

@article{Kuchner2010CollisionalGM,
  title={Collisional Grooming Models of the Kuiper Belt Dust Cloud},
  author={Marc J. Kuchner and Christopher C. Stark},
  journal={The Astronomical Journal},
  year={2010},
  volume={140},
  pages={1007-1019}
}
We modeled the three-dimensional structure of the Kuiper Belt (KB) dust cloud at four different dust production rates, incorporating both planet-dust interactions and grain-grain collisions using the collisional grooming algorithm. Simulated images of a model with a face-on optical depth of {approx}10{sup -4} primarily show an azimuthally symmetric ring at 40-47 AU in submillimeter and infrared wavelengths; this ring is associated with the cold classical KB. For models with lower optical depths… Expand

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