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Unrecognized action
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My Personal Data
My Work
Few massive bodies, one disk, how many possibilities ?
My Links
Readings
Authors |
Method |
Mass ratio |
Planet eccentricity |
Migration |
Notes |
\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 |
%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. |
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Topic revision: r4 - 2006-12-14 - RemyReche