Centre for Astrophysics, University of Central Lancashire, Preston PR1 2HE; Department of Physics, Keele University, Keele ST5 5BG
Abstract:
We present a phase-resolved ROSAT HRI X-ray light curve of the dwarf nova OY Car in quiescence. The X-ray flux is eclipsed at the same time as the optical eclipse of the primary, and the region of X-ray emission is comparable in size to the white dwarf. We use subsequent optical observations to update the orbital ephemeris of the system.