Virtual Servers

Models

Contact | Home

 

WM-basic

Fluxes

Support

Method

Remarks

 

  EUV-Fluxes of Hot Stars
New Method | Previous Method

                  

For the computation of the models presented here the method described by Pauldrach et al., 1998 has been used.

Model Grids based on different metallicities:


As an example of the fluxes that are offered for download above we show the EUV (blocking) spectrum of a supergiant with

Teff = 50000 K and log g = 3.8

spectrum of 50 kK supergiant

top

 

 
 

Last updated December 20, 1999