On the filtering and processing of dust by planetesimals - I. Derivation of collision probabilities for non-drifting planetesimals

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Fig. 7

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Contour plot of the decimal logarithm of the eccentricity focusing factors f_e (see Eq. (70)) (in black) and f_e,i (see Eq. (78)) (in red) as a function of orbital distance in a MMSN disk for dust of 1 mm in size. The eccentricity is the same as in Fig. 2.

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