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[vsnet-alert 1695] Rapid fading of T Leo

Rapid fading of T Leo

  The SU UMa-type dwarf nova T Leo is rapidly fading from the recent
anomalous superoutburst (preceded by a well-separated precursor etc.).
Intensive observations are encouraged to follow the post-superoutburst
state.

  YYMMDD(UT)   mag  observer
  980417.401   106  (R. Stubbings)
  980417.520   108  (P. Nelson)
  980417.883   115  (G. Poyner)
  980418.414   110  (R. Stubbings)
  980418.569   116  (P. Nelson)
  980418.662   113  (T. Watanabe)
  980418.887   117  (R. J. Bouma)
  980418.962   125  (G. Poyner)
  980419.246   128  (G. Hanson)
  980419.465   130  (S. Takahashi)
  980419.476   128  (T. Watanabe)
  980419.531  <110  (H. Maehara)

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