  We present JHK photometry and spectroscopy of RX J0019.8+2156. The spectrum
appears to be dominated by the accretion disc to at least 2.4 microns, over any
other source of emission. We find Paschen, Brackett and HeII lines strongly in
emission, but no HeI. There are satellite lines approximately 850km/s either
side of the strongest, unblended hydrogen lines. These satellite lines may be
the spectral signature of jets from the accretion disc.
