The grain dynamics and structures of debris discs

Details The grain dynamics and structures of debris discs The grain dynamics and structures of debris discs

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epjwc..1605006y&link_type=abstract

Research, Science and Technology of Brown Dwarfs and Exoplanets: Proceedings of an International Conference held in Shangai on O

Physics

Scientific paper

Numerical simulations are used to construct the possible dynamical
models of the Vega's debris disc. New dust grains are assumed to be
generated from two clumpy regions. The goal is to test whether an
overall circular-symmetric structure can be constructed if the birth
places of grains are not uniformly distributed in a ring region.

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