Figure 9 from Geometric Cross Sections of Dust Aggregates and a Compression Model for Aggregate Collisions

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Geometric Cross Sections of Dust Aggregates and a Compression Model for Aggregate Collisions

Authors: Toru Suyama, Koji Wada, Hidekazu Tanaka, and Satoshi Okuzumi

Suyama et al. 2012 The Astrophysical Journal 753 115.

Provider: AAS Journals

Caption: Figure 9.

Evolution of the gyration radius r _g calculated with the refined compression model. The model curves are plotted with dashed lines. The parameters are set as b = 0.15 and b′ = 3 b. The model curves agree well with the numerical results (solid lines) for all size ranges in all cases.

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