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[vsnet-alert 2238] VW CrB likely superoutburst



VW CrB likely superoutburst

   The SU UMa-type dwarf nova VW CrB (former Var21 CrB) is reported to be
in bright outburst.

  YYMMDD(UT)   mag  observer
  980913.769  <145  (T. Kinnunen)
  980914.806  <172  (L. T. Jensen, CCD unfiltered)
  980915.844  <172  (L. T. Jensen, CCD unfiltered)
  980916.844  <172  (L. T. Jensen, CCD unfiltered)
  980919.842  <152  (G. Poyner)
  980920.840  <148  (G. Poyner)
  980922.790  <145  (T. Kinnunen)
  980923.800  <151  (T. Kinnunen)
  980924.760  <151  (T. Kinnunen)
  980925.740   145  (T. Kinnunen)

   The object was originally discovered by S. V. Antipin (IBVS 4343) as
a dwarf nova.  An outburst was subsequently detected by M. Iida in 1996
June.  In 1997 May, T. Vanmunster detected a bright outburst (mag 14.1,
CVC 137, vsnet-alert 887).  CCD observations by R. Novak revealed the
existence of superhumps (vsnet-alert 892), confirming the SU UMa-type
nature of the object.  The present outburst is the first reported one
since the 1996 August normal outburst (Jensen).

Related articles:

http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/var21crb.html
http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/var21crb9606.html
http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/var21crb9705.html

Regards,
Taichi Kato

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