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An analysis of high-resolution VLT/UVES spectra of two B-type main sequencestars, NGC 346-11 and AV 304, in the Small Magellanic Cloud (SMC), has beenundertaken, using the non-LTE TLUSTY model atmospheres to derive the stellarparameters and chemical compositions of each star. The chemical compositions ofthe two stars are in reasonable agreement. Moreover, our stellar analysisagrees well with earlier analyses of H II regions. The results derived hereshould be representative of the current base-line chemical composition of theSMC interstellar medium as derived from B-type stars.Comment: 10 pages, 4 figures, 1 online tabl

A non-LTE analysis of the spectra of two narrow lined main sequence stars in the SMC