According to IAUC No. 6772, the new cataclysmic variable in Peg (reported in IAUC 6746) is again reported to be in outburst. The Beijing Astronomical Observatory supernova survey team reports the object at R=15.0 on Nov. 14.44. A search for superhumps during the current bright outburst is highly encouraged (cf. the following vsnet-alert posting) Regards, Taichi Kato (http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-alert/msg01223.html) > [vsnet-alert 1223] Apparent new dwarf nova in Peg > > IAUC No. 6746 tells the discovery of a new cataclysmic variable, apparently > a new dwarf nova, by the Qiu et al. (Beijing Astronomical Observatory team). > The object was spectroscopically confirmed as a cataclysmic variable (dwarf > nova) in outburst. > > Position: > 21h 12m 29s.54 (J2000.0) > +12o 32' 06".5 > > According to their report, the outburst was detected on Sep. 20.52 UT > at R=16.0 (<18.0 on Sep. 18), then the object faded to R=17.3 on Sep. 21.49. > > The speed of decline (1.3mag/day) strongly suggests that the object is > an SU UMa-type dwarf nova. Systematic monitoring of future outbursts and > possible superoutbursts is recommended. > > Regards, > Taichi Kato