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: Z=1.0 * Z-solar Z=0.2 * Z-solar 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 top
	Last updated December 20, 1999