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NASA NTRS · 20210003868

Disk Tides and Accretion Runaway

Hahn, J.M.·Ward, W.R.
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Abstract

It is suggested that tidal interaction of an accreting planetary embryo with the gaseous pre-planetary disk may provide a mechanism to breach the so-called runaway limit during the formation of the giant planet cores.

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BibTeXRIS

Hahn, J.M., Ward, W.R.. 1995-01-01. Disk Tides and Accretion Runaway. https://ntrs.nasa.gov/citations/20210003868

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