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[vsnet-campaign-dn 3649] V2527 Oph: further fading

V2527 Oph: further fading

   We have analyzed V2527 Oph observations by Tanabe-san (VSNET Okayama
Station).  V2527 Oph was recored by 0.9 mag fainter on May 8 than on May 5,
indicating a further fading.  There were noticeable variations in the
May 8 data.  Although we need to more analyze the remaining Kyoto
(and other) data, it is most likely that the outburst of V2527 Oph is
almost over.  The fading rate was slower than that of normal outbursts
of SU UMa-type dwarf novae.  This object needs further clarification
for its dwarf nova classification.

Regards,
Taichi Kato
VSNET Collaboration team

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