In situ formation and dynamical evolution of hot Jupiter systems
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LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements.The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planetsHATS-22b, HATS-23b and HATS-24b: three new transiting super-Jupiters from the HATSouth projectExoplanetary Science: An OverviewA deeper view of the CoRoT-9 planetary system
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In situ formation and dynamical evolution of hot Jupiter systems
description
article publié dans la revue scientifique Astrophysical Journal
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im September 2016 veröffentlichter wissenschaftlicher Artikel
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scientific article published in the Astrophysical Journal
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wetenschappelijk artikel
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наукова стаття, опублікована у вересні 2016
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name
IN SITU FORMATION AND DYNAMICAL EVOLUTION OF HOT JUPITER SYSTEMS
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In situ formation and dynamical evolution of hot Jupiter systems
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type
label
IN SITU FORMATION AND DYNAMICAL EVOLUTION OF HOT JUPITER SYSTEMS
@nl
In situ formation and dynamical evolution of hot Jupiter systems
@en
prefLabel
IN SITU FORMATION AND DYNAMICAL EVOLUTION OF HOT JUPITER SYSTEMS
@nl
In situ formation and dynamical evolution of hot Jupiter systems
@en
P2093
P356
P1476
In situ formation and dynamical evolution of hot Jupiter systems
@en
P2093
Gregory P. Laughlin
Konstantin Batygin
Peter H. Bodenheimer
P304
P356
10.3847/0004-637X/829/2/114
P407
P577
2016-09-28T00:00:00Z
P818
1511.09157
P819
2016ApJ...829..114B