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[ABRIDGED] Metal-rich globular clusters provide important tracers of theformation of our Galaxy. Moreover, and not less important, they are veryimportant calibrators for the derivation of properties of extra-galacticmetal-rich stellar populations. Nonetheless, only a few of the metal-richglobular clusters in the Milky Way have been studied using high-resolutionstellar spectra to derive elemental abundances. In this paper we presentelemental abundances for nine HB stars in the metal-rich globular clusterNGC6352. The elemental abundances are based on high-resolution, highsignal-to-noise spectra obtained with VLT/UVES. The elemental abundances havebeen derived using standard LTE calculations. We find that NGC6352 has [Fe/H]=-0.55, is enhanced in the alpha-elements to about +0.2 dex for Ca, Si, and Tirelative to Fe. For the iron-peak elements we find solar values. Based on thespectroscopically derived stellar parameters we find that an E(B-V)=0.24 and(m-M) roughly equal to 14.05 better fits the data than the nominal values. Aninvestigation of log(gf)-values for suitable FeI lines lead us to theconclusion that the commonly used correction to the May et al.(1974) datashould not be employed. Note: only the postscript reproduces the finding chartcorrectly.

Stellar abundances and ages for metal-rich Milky Way globular clusters - Stellar parameters and elemental abundances for 9 HB stars in NGC6352