Origin and early evolution of the planet
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D. MΓΆhlmann
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Article
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1985
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Springer Netherlands
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English
β 706 KB
It is shown by linear stability analysis that a preplanetary (presatellite) disk of dust and gas with Keplerian velocity field can become unstable due to the collective self-gravity of the disk. The radial distribution of rings, which may result from this instability, is derived. These rings later o