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[vsnet-alert 7269] RX J1155.4-5641: new SU UMa star



RX J1155.4-5641: new SU UMa star

   We have received a report that Berto Monard has confirmed superhumps
with a period of 0.0622 d (cf. vsnet-alert 7264).  The object is now
established as a genuine SU UMa-type dwarf nova.  Since the superhump
period is relatively short in spite of the low outburst amplitude
and relatively frequent outbursts, the star may be something relatively
exceptional among short-period SU UMa systems.  Further observations
are strongly encouraged.

Regards,
Taichi Kato
VSNET Collaboration team

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