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Article Contents
1 Introduction
2 The ultraviolet spectra of the Pop II A-type stars
3 The models
4 The dependence of the ultraviolet spectral energy distribution on $\vec{T}_\mathsf{eff}$, log$\vec{g}$ and metallicity
5 The fitting procedure
6 Parameters from the visible energy distribution for some stars of the sample
7 The effect of reddening, metallicity, microturbulent velocity and convection on the parameters
8 Comparison of $\vec{T}_\mathsf{eff}$ and log$\vec{g}$ with other determinations and with the evolutionary models
9 Conclusions
Appendix A: Comparison of the IUE fluxes of the Pop II A-type stars with the computed fluxes
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Copyright ESO 2001
Published by EDP Sciences