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Fig. 10


Same as in Fig. 9, but for asteroid (161989) Cacus. The solid curves show the theoretical dependence for three values of the bulk density ρb = 2 g cm-3, 2.5 g cm-3, and 3 g cm-3 (see the labels). The gray vertical zone indicates plausible range of Γ, the dark gray the best-fit values (Sec. 2.3). The horizontal gray area is the Yarkovsky da/ dt secular value from the orbit determination (1σ interval).

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