Disk dynamics and planet migration
We review models of protoplanetary disks. In the earlier stages of evolution, disks are subject to gravitational instabilities that redistribute mass and angular momentum on short timescales. Later on, when the mass of the disk is below ten percent or so of that of the central star, accretion occurs...
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| Formaat: | Journal article |
| Taal: | English |
| Gepubliceerd in: |
2010
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