The formation of a gas giant planet in a viscously evolved protoplanetary disk within the core accretion model
Sign Up to like & getrecommendations! Published in 2018 at "Astrophysics and Space Science"
DOI: 10.1007/s10509-018-3406-y
Abstract: The gas giant planets’ formation processes in a viscously evolved protoplanetary disk are studied in the context of the core accretion model. In this paper, we follow the entire formation process of the core accretion… read more here.
Keywords: disk; core; accretion; gas ... See more keywords
Filling in the gaps: Can gravitationally unstable discs form the seeds of gas giant planets?
Sign Up to like & getrecommendations! Published in 2023 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stad1564
Abstract: Circumstellar discs likely have a short window when they are self-gravitating and prone to the effects of disc instability, but during this time the seeds of planet formation can be sown. It has long been… read more here.
Keywords: gas; form; gas giant; planet formation ... See more keywords
Zero age planetary orbit of gas giant planets revisited: reinforcement of the link with stellar metallicity
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DOI: 10.1093/mnras/stw2592
Abstract: In 2005 we suggested a relation between the optimal locus of gas giant planet formation, prior to migration, and the metallicity of the host star, based on the core accretion model and radial profiles of… read more here.
Keywords: gas; age planetary; planetary orbit; giant planets ... See more keywords
Direct imaging and astrometric detection of a gas giant planet orbiting an accelerating star
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DOI: 10.1126/science.abo6192
Abstract: Direct imaging of gas giant exoplanets provides information on their atmospheres and the architectures of planetary systems. However, few planets have been detected in blind surveys with direct imaging. Using astrometry from the Gaia and… read more here.
Keywords: star; direct imaging; gas giant; detection ... See more keywords