This page offers full insight into one typical T Tauri ProDiMo model.
The parameters of this model are chosen to roughly match the continuum and line fluxes of real class II T Tauri stars.
You can download here
- html-presentation: This page gets you started, gives an overview of the model setup, the underlying ideas, and the capabilities of ProDiMo to predict continuum and line observations
- TypicalModel.pdf: download the html-presentation as pdf document
- full graphical output (153 pages): most (but not all) of the output data visualized
- numerical output files: download this zip-file to study the full information: densities, temperatures, chemical composition, internal radiation field, individual heating/cooling rates, calculated SED, line fluxes, line profiles, line maps, etc.
Please contact us if you have any questions, comments, or would like to collaborate.
An example TTauri ProDiMo model
The following ProDiMo model of a “typical TTauri star” is designed to predict continuum and line fluxes that roughly resemble the observations of real class II TTauri stars. The effective stellar temperature is chosen as Teff = 4000 K, and the stellar luminosity L✶ = 1 L☉; these values correspond to spectral type K7, a stellar mass of M✶ = 0.7 M☉ and an age of about 1.6 Myrs.
See all chapters:
1. Spectral Energy Distribution
2. Disc Shape and Dust Settling
3. Gas and Dust Temperatures
4. Chemical Structure
5. Predicted Continuum Observations
6. Predicted Line Observations