Non-symmetrical protoplanetary disks destroyed by UV photoevaporation
Abstract
We have developed geometric disk models to study the circumstellar geometries by fitting the spectral energy distribution (SED) of T Tauri and Herbig Ae/Be stars. The simulations provide means to recognize the signatures of different disk structures, including the effects due to external UV photoevaporation.
- Publication:
-
Triggered Star Formation in a Turbulent ISM
- Pub Date:
- 2007
- DOI:
- 10.1017/S174392130700213X
- Bibcode:
- 2007IAUS..237..425H
- Keywords:
-
- ISM: Orion clouds;
- Stars: pre-main sequence;
- Method: genetic algorithms