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Friends of hot Jupiters. IV. Stellar companions beyond 50 AU might facilitate giant planet formation, but most are unlikely to cause Kozai–lidov migration

H Ngo, HA Knutson, S Hinkley, M Bryan… - The Astrophysical …, 2016 - iopscience.iop.org
Stellar companions can influence the formation and evolution of planetary systems, but there
are currently few observational constraints on the properties of planet-hosting binary star …
被引用次数：160 相关文章
[PDF] researchgate.net

[PDF][PDF] FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 AU MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO …

H Ngo, HA Knutson, S Hinkley, M Bryan… - arXiv preprint arXiv …, 2016 - researchgate.net
Stellar companions can influence the formation and evolution of planetary systems, but there
are currently few observational constraints on the properties of planet-hosting binary star …
[PDF] archive.org

[PDF][PDF] FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 AU MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO …

H Ngo, HA Knutson, S Hinkley, M Bryan… - arXiv preprint arXiv …, 2016 - scholar.archive.org
Stellar companions can influence the formation and evolution of planetary systems, but there
are currently few observational constraints on the properties of planet-hosting binary star …
[PDF] caltech.edu

[PDF][PDF] FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 AU MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO …

H Ngo, HA Knutson, S Hinkley… - arXiv preprint …, 2016 - authors.library.caltech.edu
Stellar companions can influence the formation and evolution of planetary systems, but there
are currently few observational constraints on the properties of planet-hosting binary star …

Friends of Hot Jupiters. IV. Stellar Companions Beyond 50 au Might Facilitate Giant Planet Formation, but Most are Unlikely to Cause Kozai-Lidov Migration

H Ngo, HA Knutson, S Hinkley, M Bryan… - The Astrophysical …, 2016 - ui.adsabs.harvard.edu
Stellar companions can influence the formation and evolution of planetary systems, but there
are currently few observational constraints on the properties of planet-hosting binary star …

Friends of Hot Jupiters. IV. Stellar companions beyond 50 AU might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration

H Ngo, HA Knutson, S Hinkley, M Bryan… - arXiv preprint arXiv …, 2016 - arxiv.org
Stellar companions can influence the formation and evolution of planetary systems, but there
are currently few observational constraints on the properties of planet-hosting binary star …

Friends of hot Jupiters. IV. Stellar companions beyond 50 au might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration

H Ngo, S Hinkley, M Bryan, K Batygin… - Astrophysical …, 2016 - open.bu.edu
Stellar companions can influence the formation and evolution of planetary systems, but there
are currently few observational constraints on the properties of planet-hosting binary star …

FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO …

H Ngo, HA Knutson, S Hinkley, M Bryan, JR Crepp… - 2016 - repository.arizona.edu
Stellar companions can influence the formation and evolution of planetary systems, but there
are currently few observational constraints on the properties of planet-hosting binary star …

[引用][C] FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO …

H Ngo, HA Knutson, S Hinkley, M Bryan… - The Astrophysical …, 2016 - cir.nii.ac.jp
FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT
FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO CAUSE KOZAI–LIDOV …
[PDF] core.ac.uk

[PDF][PDF] FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO …

H Ngo, HA Knutson, S Hinkley, M Bryan… - The Astrophysical …, 2016 - core.ac.uk
Stellar companions can influence the formation and evolution of planetary systems, but there
are currently few observational constraints on the properties of planet-hosting binary star …