Hot Jupiters from Disruption of Resonant Chains in Postdisk Evolution
The formation of hot Jupiters has been a subject of interest in the field of exoplanet science. According to conventional scenarios, these gas giants are believed to form beyond the snow line and subsequently migrate inward. Although the early formation history of hot Jupiters is not well understood...
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Published in | The Astronomical journal Vol. 166; no. 6; pp. 267 - 273 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Madison
The American Astronomical Society
01.12.2023
IOP Publishing |
Subjects | |
Online Access | Get full text |
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