there is a spectrum of BC UMa at minimum in Mukai, K., Mason, K.O., Howell, S.B., Allington-Smith, J., Callanan, P.J., Charles, P.A., Hassall, B.J.M., Machin, G., Naylor, T., Smale, A.P., and van Paradijs, J. (1990). "Spectroscopy of Faint Cataclysmic Variable Candidates," MNRAS, 245, 385. This system is one of only two or three known DN which show spectral lines from the white dwarf in the optical spectrum. WZ Sge is another. Steve B. Howell Planetary Science Institute, Astrophysics Group 620 N. 6th Ave. Tucson, AZ 85705 USA Phone (520) 622-6300 Fax (520) 622-8060 e-mail: howell@frankenstein.psi.edu homepage: http://vsnet.psi.edu/