[vsnet-outburst 9002] HS Vir relatively bright outburst

[Taichi Kato]

    According to Rod Stubbings, the SU UMa-type dwarf nova HS Vir
is undergoing a relatively bright outburst (possibly a superoutburst).
The last superoutburst was in 2007 March-April (max 13.5).

  YYYYMMDD(UT)   mag  observer
  20080520.1114 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080522.1139 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080529.517   139  (Rod Stubbings)