Note that this homepage makes use of popup windows; a popup blocker
prevents its proper operation.
In case of problems please contact Wolf-Rainer Hamann
This WEB interface has been developed by Daniel M. Hamann and Wolf-Rainer Hamann (2004).
The following data are available for each model:
- Spectral Energy Distribution
(emergent flux received at 10pc distance, low spectral resolution)
- Line spectrum in high resolution for different wavelength bands
(optionally normalized or flux-calibrated)
Model parameters and organisation
The models are arranged in different Model Grids.
Each model grid is characterized by a set of common parameters, such as
stellar luminosity, terminal wind velocity, clumping contrast, and
chemical composition. The following grids are available yet:
|log L / Lsun||5.3||5.3||5.3|
New (August 2012): The WNL grid has been re-calculated in 2012 and is now shown by default. Details of the new version are given here. The previous version of the WNL grid can still be accessed by choosing "WNL-2004" in the drop-down menu below.
New (May 2013): The WNE grid has been re-calculated in 2013 and is now shown by default. Details of the new version are given here. The previous version of the WNE grid can still be accessed by choosing "WNE-2004" in the drop-down menu below.