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Turbulent Torques on Protoplanets in a Dead Zone
ASTROPHYSICAL JOURNAL, no. 1 (2007): 805-819
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Migration of protoplanets in their gaseous host disks may be largely responsible for the observed orbital distribution of extrasolar planets. Recent simulations have shown that themagnetorotational turbulence thought to drive accretion in protoplanetary disks can affect migration by turning it into an orbital random walk. However, these s...更多
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