Free Access

Fig. 1

image

D vs. Γ for near-Earth and main belt asteroids of S, C, B, X, and E types and dynamical classes with D < 100 km. The data arefit to the function y = a xb shown as the dark line using orthogonal distance regression (Boggs & Rogers 1990). Measurements of D and Γ are taken from Delbó et al. (2003), Lamy et al. (2008), Delbo & Tanga (2009), Masiero et al. (2011), Müller et al. (2011), Wolters et al. (2011), Marchis et al. (2012), Müller et al. (2012), Müller et al. (2013), Emery et al. (2014), Alí-Lagoa et al. (2014), Müller et al. (2014b), Rozitis & Green (2014), Hanuš et al. (2015), Naidu et al. (2015), Hanuš et al. (2016).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.