Self-gravitating planetary envelopes and the core-nucleated instability
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DOI: 10.1093/mnras/stz2796
Abstract: Planet formation scenarios can be constrained by the ratio of the gaseous envelope mass relative to the solid core mass in the observed exoplanet populations. One-dimensional calculations find a critical (maximal) core mass for quasi-static… read more here.
Keywords: core nucleated; gravitating planetary; self gravitating; nucleated instability ... See more keywords