On the formation of super-Jupiters: core accretion or gravitational instability?

The Core Accretion model is widely accepted as the primary mechanism for forming planets up to a few Jupiter masses. However, the formation of super-massive planets remains a subject of debate, as their formation via the Core Accretion model requires super-solar metallicities. Assuming stellar atmos...

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Vydané v:	Astrophysics and space science Ročník 369; číslo 12; s. 122
Hlavní autori:	Nguyen, Max, Adibekyan, Vardan
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	Dordrecht Springer Netherlands 01.12.2024 Springer Nature B.V
Predmet:	Accretion Accretion disks Astrobiology Astronomy Astrophysics and Astroparticles Building materials Cosmology Extrasolar planets Gas giant planets Gravitational instability Jupiter Jupiter atmosphere Metal content Metallicity Observations and Techniques Physics Physics and Astronomy Planet formation Planetary composition Planetary mass Planets Protoplanetary disks Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Stellar atmospheres Stellar mass Stellar mass accretion Chemical abundances Exoplanet formation Planet hosting stars Methods: statistical
ISSN:	0004-640X, 1572-946X
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