Browsing Research Articles by Subject "Accretion discs"
Now showing items 1-5 of 5
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Are the observed gaps in protoplanetary discs caused by growing planets?
(Monthly Notices of the Royal Astronomical Society, 2019)Recent detailed observations of protoplanetary discs revealed a lot of substructures that are mostly ring like. One interpretation is that these rings are caused by growing planets. These potential planets are not yet ... -
Are the observed gaps in protoplanetary discs caused by growing planets?
(Monthly Notices of the Royal Astronomical Society, 2019-07-10)Recent detailed observations of protoplanetary discs revealed a lot of substructures that are mostly ring like. One interpretation is that these rings are caused by growing planets. These potential planets are not yet ... -
Are the observed gaps in protoplanetary discs caused by growing planets?
(Royal Astronomical Society, 2019-06)Recent detailed observations of protoplanetary discs revealed a lot of substructures that are mostly ring like. One interpretation is that these rings are caused by growing planets. These potential planets are not yet ... -
Planet population synthesis driven by pebble accretion in cluster environments
(Oxford University Press on behalf of the Royal Astronomical Society, 2016-12)The evolution of protoplanetary discs embedded in stellar clusters depends on the age and the stellar density in which they are embedded. Stellar clusters of young age and high stellar surface density destroy protoplanetary ... -
Probing the impact of varied migration and gas accretion rates for the formation of giant planets in the pebble accretion scenario
(Monthly Notices of the Royal Astronomical Society, 2020)The final orbital position of growing planets is determined by their migration speed, which is essentially set by the planetary mass. Small mass planets migrate in type-I migration, while more massive planets migrate in ...