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

Tristan Guillot; Shigeru Ida; Chris W. Ormel

doi:10.1051/0004-6361/201323021

Home

All issues

Volume 572 (December 2014)

A&A, 572 (2014) A72

Full HTML

Free Access

Fig. 7

Open with DEXTER Download original image

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.

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.