Hydrodynamics of embedded planets’ first atmospheres – III. The role of radiation transport for super-Earth planets

Abstract The population of close-in super-Earths, with gas mass fractions of up to 10 per cent represents a challenge for planet formation theory: how did they avoid runaway gas accretion and collapsing to hot Jupiters despite their core masses being in the critical range of M c ≃ 10 M⊕? Previous th...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2017-11, Vol.471 (4), p.4662-4676
Hauptverfasser:	Cimerman, Nicolas P., Kuiper, Rolf, Ormel, Chris W.
Format:	Artikel
Sprache:	eng
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