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My Personal Data

E-mail remy.reche@univ-grenoble-alpes.fr

My Work

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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Topic revision: r4 - 2006-12-14 - RemyReche
 
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