[vsnet-alert 3726] TmzV36 fading

[Taichi Kato <tkato>]

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

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