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[vsnet-campaign-dn 2243] 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
vsnet-adm@kusastro.kyoto-u.ac.jp
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
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