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We have performed abundance analysis of two slowly rotating, late A-typestars, HD 32115 (HR 1613) and HD 37594 (HR 1940), based on obtained echellespectra covering the spectral range 4000-9850 AAngstrom. These spectra allowedus to identify an extensive line list for 31 chemical elements, the mostcomplete to date for A-type stars. Two approaches to abundance analysis wereused, namely a ``manual'' (interactive) and a semi-automatic procedure forcomparison of synthetic and observed spectra and equivalent widths. For someelements non-LTE (NLTE) calculations were carried out and the correspondingcorrections have been applied. The abundance pattern of HD 32115 was found tobe very close to the solar abundance pattern, and thus may be used as anabundance standard for chemical composition studies in middle and late A stars.Further, its H-alpha line profile shows no core-to-wing anomaly like that foundfor cool Ap stars and therefore also may be used as a standard in comparativestudies of the atmospheric structures of cool, slowly rotating Ap stars. HD37594 shows a metal deficiency at the level of -0.3 dex for most elements andtriangle-like cores of spectral lines. This star most probably belongs to theDelta Scuti group.Comment: 10 pages, 4 figure

Abundance analysis of two late A-type stars HD 32115 and HD 37594