STScI NRDD, 20 Oct 2005
Dynamics and Structure in Resolved Dusty Disks. Pawel Artymowicz University of Toronto. 1. Structures vs. reasons (planets,…) 2. Dust, avalanches, f IR , gas, and the calssification of disks 3. HD 141569A 4. Non-axisymmetric features without planets. STScI NRDD, 20 Oct 2005. New edge-
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