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Identifying Collisional Families in the Kuiper Belt

  • Authors: Robert A. Marcus, Darin Ragozzine, Ruth A. Murray-Clay, and Matthew J. Holman

Marcus et al. 2011 The Astrophysical Journal 733 40.

  • Provider: AAS Journals

Caption: Figure 11.

Ratio of family members, N fam to the square root of the number of background objects, , with Δ v minv esc vs. (a) size of the progenitor and (b) inclination of the progenitor. In panel (a), symbol type indicates the subpopulation to which the progenitor belonged: triangles—cold classicals, squares—hot classicals, diamonds—inner classicals. The lines show N fam/ N bg ~ R 2. In panel (b), symbol indicates the radius of the progenitor: triangles— R ⩾ 400 km, squares—300 km ⩽ R < 400 km, diamonds—200 km ⩽ R < 300 km, circles— R ⩽ 200 km.

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