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- W2964339675 abstract "We present preliminary results on the ability of self‐gravitating disks to cool in response to their internal heating. These disks are modelled using a smoothed particle hydrodynamics (SPH) code with radiative transfer [1], and we investigate the ability of these disks to maintain a state of thermal equilibrium with their boundaries as an indication of their likelihood to fragment." @default.
- W2964339675 created "2019-07-30" @default.
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- W2964339675 date "2009-01-01" @default.
- W2964339675 modified "2023-10-16" @default.
- W2964339675 title "Self-gravitating disks with Radiative Transfer: Their role in Giant Planet Formation" @default.
- W2964339675 doi "https://doi.org/10.1063/1.3215821" @default.
- W2964339675 hasPublicationYear "2009" @default.
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