NY Ser more information Additional information on this target, extracted from previous vsnet-alert messages: ----------------------------------------------------------------------------- (vsnet-alert 397, 1996 Apr. 23) > Dear Colleagues, > > Our observation revealed that the ongoing outburst in PG 1510+234 > (=NSV06990 = Ser1 in Downes & Shara(1993)) has been lasting for at > least three days and the superhumps with an amplitude of ~0.3 mag > clearly exist on April 23. Although the superhump period can not > be measured precisely due to shortness of the coverage, it seems > to exceed 2 hours. It was proved that PG 1510+234 is an SU UMa-type > dwarf nova with a small amplitude of ~3mag. > > Best regards, > Daisaku Nogami & Ouda Team (vsnet-alert 398) > Dear Colleagues, > > We have just reduced the PG1510+234 data obtained in the last > night. The superhumps with an amplitude of ~0.3 mag still > existed. Surprisingly, our period analysis using the April 23 > and 24 results gives the superhump period of 0.1064 (+-0.0003) > day (= 153.2 (+-0.4) min)! Is PG 1510+234 located at the midst > of the CV period gap?! > > Best regards, > Daisaku Nogami & Ouda Team ----------------------------------------------------------------------------- The full paper, with detailed long-term photometry, by D. Nogami et al. is available at http://ftp.kusastro.kyoto-u.ac.jp/pub/vsnet/preprints/NY_Ser and the preceding paper on outburst activity information http://ftp.kusastro.kyoto-u.ac.jp/pub/vsnet/preprints/PG1510+234 VSNET NY Ser page: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/pg1510.html Regards, Taichi Kato