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Keywords:

  • accretion, accretion discs;
  • binaries: close;
  • stars: individual: RE J1255+266;
  • stars: low-mass, brown dwarfs;
  • novae, cataclysmic variables;
  • X-rays: stars

We present a previously unpublished ROSAT Wide Field Camera observation of the transient source RE J1255+266 made just 4 d before the discovery observations. The source is not detected, limiting the duration of the outburst to be less than expected for a superoutburst of a WZ Sge system.

We also present a marginal detection of X-ray emission from RE J1255+266 using ASCA. The most probable luminosity is 6×1029 erg s−1, which is very similar to WZ Sge itself.

We discuss the nature of the source in the light of these observations, and conclude that it is most probably a WZ Sge system, but that the observed outburst must have been a normal dwarf nova outburst.