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Few massive bodies, one disk, how many possibilities ?

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Readings

Authors	Method	Mass ratio	Planet eccentricity	Migration	Notes
%EMBEDBIB{webname="RemyReche" style="string" bibfile="biblio.bib" sort="string" select1="author (Wyatt)" select2="year (2003)}%	semi-analytic		0	planet
\citet{2006ApJ...639.1153W}	semi-analytic			none	This work extends the precedent one to smaller particles sensitive to pression radiation.
\citet{2003ApJ...588.1110K}	analytic	0.001 to 15	0 to 0.6	particles	Only resonant particles trapped during migration due to P-R drag.
\citet{2005ApJ...625..398D}	numerical	0.01 to 3	0 to 0.7	particles	Particles migrate due to P-R drag and solar wind.
\citet{2002AJ....124.2305M}	numerical			particles	Study of the Kuiper Belt.
Our paper in prep.	numerical	0.001 to 2	0 to 0.7	planet	Only planetesimals disk

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