KV Dra rare outburst As Mike Simonsen reported, the SU UMa-type dwarf nova KV Dra (RX J1450.5+6403) is reported to be in outburst. The object underwent an superoutburst in 2000 May (see vsnet-alert 4858 and Nogami et al. 2000 A&A 364, 701). However, only two normal outbursts have been reported since then. The outburst frequency of this object may be low. Kato et al. (2001) PASJ 53, 1191 wrote: > System with a short orbital period (Porb = 0.05898 d, > P_SH = 0.0601 d). Nogami et al. (2000) suggested the object to be > an intermediate object between WZ Sge-type and ER UMa-type stars. > One well-established superoutburst in 2000 May and subsequent normal > outbursts are known. The lack of further outbursts (VSNET) may suggest > a lower typical frequency of outbursts than proposed by > Nogami et al. Kato et al. (2000) reported double-wave modulations > in quiescence, which are reminiscent of those of WZ Sge. > More observations are needed to establish the outburst behavior and > the evolution of superhumps. Although the present magnitude is fainter than the 2000 superoutburst, please observe KV Dra as intensively as possible! Regards, Taichi Kato VSNET Collaboration team