SEDs of flared dust disks: radiation transfer model versus two-layer model
| dc.creator | Kraus, M. | |
| dc.date | 2003-05-28 | |
| dc.date.accessioned | 2026-07-07T02:08:37Z | |
| dc.date.available | 2026-07-07T02:08:37Z | |
| dc.description | A radiation transfer model for the top-layer of a flared dust disk around a low mass star is presented. The disk structure, temperature distribution and spectral energy distribution are compared with the results of the analytical two-layer model of Chiang & Goldreich. We find that both, a proper iterative calculation of the main parameters and proper radiation transfer calculations, are important to not overestimate the disk structure and its emission especially at long wavelengths. | |
| dc.description | 8 pages, 5 figures, to appear in conference proceedings of Open Issues in Local Star Formation and Early Stellar Evolution | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0305532 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0305532 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6119 | |
| dc.subject | Astrophysics | |
| dc.title | SEDs of flared dust disks: radiation transfer model versus two-layer model | |
| dc.type | text |