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• W3103292495 abstract "Context. The formation of resonant planet pairs in exoplanetary systems involves planetary migration inside the protoplanetary disc. After a resonant capture, subsequent migration leads to a large increase in planetary eccentricities, if no damping mechanism is applied. This has led to the conclusion that the migration of resonant planetary systems cannot take place across large radial distances, but must be terminated rapidly by disc dissipation." @default.
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• W3103292495 date "2008-03-19" @default.
• W3103292495 modified "2023-10-17" @default.
• W3103292495 title "Influence of an inner disc on the orbital evolution of massive planets migrating in resonance" @default.
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• W3103292495 doi "https://doi.org/10.1051/0004-6361:20079291" @default.
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