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We present XMM-Newton X-ray spectra of the disc accreting cataclysmicvariable OY Car, which were obtained during the performance verification phaseof the mission. These data were taken 4 days after a short outburst. In theEPIC spectra we find strong iron Kalpha emission with weaker iron Kbetaemission together with silicon and sulphur lines. The spectra are best fittedwith a three temperature plasma model with a partial covering absorber.Multiple temperature emission is confirmed by the emission lines seen in theRGS spectrum and the H/He like intensity ratio for iron and sulphur which implytemperatures of ~7keV and ~3keV respectively.Comment: Accepted by A&A for publication in the special issue on XMM results,  4 page

First XMM-Newton observations of a Cataclysmic Variable II: The X-ray spectrum of OY Car