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[vsnet-outburst 1991] HS Vir outburst
HS Vir outburst
Ths SU UMa-type dwarf nova HS Vir is in outburst. The outburst is
relatively bright in this season, and could be a superoutburst.
The last superoutburst was observed in 2000 May, and no outbursts
brighter than 14.5 were observed since then. If the present outburst
is a superoutburst, the detection at this early epoch could provide
an excellent oppportunity for a detailed study.
YYYYMMDD(UT) mag observer
20010412.428 <140 (R. Stubbings)
20010413.446 <144 (R. Stubbings)
20010414.253 <135 (M. Simonsen)
20010416.481 140 (R. Stubbings)
Regards,
VSNET Collaboration team
vsnet-adm@kusastro.kyoto-u.ac.jp
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp