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1 Introduction
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2 The ultraviolet spectra of the Pop II A-type stars
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3 The models
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4 The dependence of the ultraviolet spectral energy distribution on
 ,
log
and metallicity
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5 The fitting procedure
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6 Parameters from the visible energy distribution for some stars of the sample
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7 The effect of reddening, metallicity, microturbulent velocity
and convection on the parameters
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8 Comparison of
and log
with other determinations and with the
evolutionary models
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9 Conclusions
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Appendix A: Comparison of the IUE fluxes of the Pop II A-type stars
with the computed fluxes
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References
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Online Material
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