RemyReche < Main

---++ My Personal Data 

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

---++ My Work 

_Few massive bodies, one disk, how many possibilities ?_

---++ My Links 

---++ Readings 

<h2>
| *Authors* | *Method* | *Mass ratio<br />* | *Planet eccentricity<br />* | *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 |

  My Personal Preferences </h2>

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This topic: Main > TWikiUsers > RemyReche
Topic revision: r4 - 2006-12-14 - RemyReche