Protoplanetary Disk Resonances and Type I Migration

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics

Scientific paper

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Details

6 pages, 3 figures, accepted by ApJ

Scientific paper

10.1088/0004-637X/741/2/109

Waves reflected by the inner edge of a protoplanetary disk are shown to
significantly modify Type I migration, even allowing the trapping of planets
near the inner disk edge for small planets in a range of disk parameters. This
may inform the distribution planets close to their central stars, as observed
by the Kepler mission.

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