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A low mass for Mars from Jupiter's early gas-driven migrationHot Jupiters from secular planet-planet interactions.Migration-induced architectures of planetary systems.Secular dynamics in hierarchical three-body systemsHalting type I planet migration in non-isothermal disksMigration of accreting planets in radiative discs from dynamical torquesConstraints on resonant-trapping for two planets embedded in a protoplanetary discTwo phase, inward-then-outward migration of Jupiter and Saturn in the gaseous solar nebulaGrowing and moving low-mass planets in non-isothermal disksRODEO: a new method for planet-disk interactionImaging the heart of astrophysical objects with optical long-baseline interferometry
P2860
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P2860
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Mai 2003 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в травні 2003
@uk
name
Runaway Migration and the Formation of Hot Jupiters
@en
Runaway Migration and the Formation of Hot Jupiters
@nl
type
label
Runaway Migration and the Formation of Hot Jupiters
@en
Runaway Migration and the Formation of Hot Jupiters
@nl
prefLabel
Runaway Migration and the Formation of Hot Jupiters
@en
Runaway Migration and the Formation of Hot Jupiters
@nl
P356
P1476
Runaway Migration and the Formation of Hot Jupiters
@en
P2093
F. S. Masset
J. C. B. Papaloizou
P304
P356
10.1086/373892
P407
P577
2003-05-01T00:00:00Z
P5875
P818
astro-ph/0301171
P819
2003ApJ...588..494M