Self-gravitating discs with radiative transfer: their role in giant planet formation
| dc.creator | Meru, Farzana | |
| dc.creator | Bate, Matthew R. | |
| dc.date | 2009-05-13 | |
| dc.date.accessioned | 2026-07-07T13:14:31Z | |
| dc.date.available | 2026-07-07T13:14:31Z | |
| dc.description | We present preliminary results on the ability of self-gravitating discs to cool in response to their internal heating. These discs are modelled using a Smoothed Particle Hydrodynamics (SPH) code with radiative transfer (Whitehouse, Bate & Monaghan 2005) and we investigate the ability of these discs to maintain a state of thermal equilibrium with their boundaries as an indication of their likelihood to fragment. | |
| dc.description | To be published in American Institute of Physics; Conference proceedings - Exoplanets and Disks: Their Formation and Diversity; 2 pages, 2 figures | |
| dc.identifier | https://arxiv.org/abs/0905.2122 | |
| dc.identifier | http://arxiv.org/abs/0905.2122 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/230232 | |
| dc.subject | Earth and Planetary Astrophysics | |
| dc.title | Self-gravitating discs with radiative transfer: their role in giant planet formation | |
| dc.type | text |