Fig. 3
Velocity distribution between two virtual NEOs following control orbits statistically compatible with those of (454100) 2013 BO73 and 2018 LA (top panel) – in the histogram, the bin width is 0.025 km s−1, with IQR = 0.194 km s−1 and a mean value of 2.6 ± 0.2 km s−1; 454100 and 2018 TU (second to top panel) – bin width is 0.053 km s−1, with IQR = 0.381 km s−1 and a mean value of 21.9 ± 0.3 km s−1; 2016 LR and 2018 LA (middle panel) – bin width is 0.029 km s−1, with IQR = 0.212 km s−1 and a mean value of 1.8 ± 1.9 km s−1; 2018 BA5 and 2018 LA (second to bottom panel) – bin width is 0.119 km s−1, with IQR = 0.859 km s−1 and a mean value of 11.8 ± 1.3 km s−1; 2018 LA and 2018 TU (bottom panel) – bin width is 0.071 km s−1, with IQR = 0.513 km s−1 and a mean value of 21.5 ± 0.4 km s−1.
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