Formation of hot Jupiters through secular chaos and dynamical tides
Sign Up to like & getrecommendations! Published in 2019 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stz1011
Abstract: The population of giant planets on short-period orbits can potentially be explained by some flavours of high-eccentricity migration. In this paper, we investigate one such mechanism involving ‘secular chaos’, in which secular interactions between at… read more here.
Keywords: dynamical tides; jupiter; planet; secular chaos ... See more keywords