2002MNRAS.334..805R

We report observations of the asynchronous polar BY Cam made using XMM-Newton . We find evidence for two accretion regions which have significantly different spectra. In both regions we find evidence for hard X-ray emission from the post-shock flow while we observe a distinct soft X-ray blackbody component in only one. We detect two emission lines in the RGS detectors which we attribute to nitrogen Nvi and Nvii: the first time that nitrogen lines have been detected in an X-ray spectrum of a cataclysmic variable. In the time interval where we observe short time-scale variability we find the hard X-ray light curve is correlated with the softest energies in the sense that the hard X-rays trail the soft X-rays and are anti-correlated. We suggest that there are a small number of dense blobs of material which impact the white dwarf without forming a shock and release an amount of optically thick material which obscures hard X-rays for a short duration.