TmzV36 fading Time-series CCD observations (M. Uemura and T. Kato) indicate that the TmzV36 is now relatively rapidly fading from the reported (rare) outburst. No apparent superhumps were detected during the 2.5-hour run on Nov. 19. The above findings together with CCD photometry reported by Schmeer seem to support the suggested dwarf nova classification of this object. The present outburst can be either a normal outburst of an SU UMa star or an outburst of SS Cyg star. Observations on the subsequent nights will be particularly useful in discriminating the possibilities. YYMMDD(UT) mag observer 991113.535 180:C (P. Schmeer) 991114.535 179C (P. Schmeer) 991117.528 147C (P. Schmeer) 991118.842 15.26C (Ouda team) 991119.693 15.82C (Ouda team) Regards, Taichi Kato Makoto Uemura Patrick Schmeer