Creating Pileups of Eccentric Planet Pairs Wide of Mean Motion Resonances through Divergent Migration

Observed pileups of planets with period ratios ≈1% wide of strong mean motion resonances (MMRs) pose an important puzzle. Early models showed that they can be created through sustained eccentricity damping, driving a slow separation of the orbits, but this picture is inconsistent with elevated eccen...

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Үндсэн зохиолчид:	Jingyun Lin, Ivan Dudiak, Samuel Hadden, Daniel Tamayo
Формат:	Artigo
Хэл сонгох:	Inglês
Хэвлэсэн:	IOP Publishing 2025-01-01
Цуврал:	The Astrophysical Journal
Нөхцлүүд:	Exoplanet formation Orbital resonances N-body simulations Transit timing variation method Exoplanet migration Exoplanet astronomy
Онлайн хандалт:	https://doi.org/10.3847/1538-4357/ae17cf
Шошгууд:	Шошго нэмэх Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!