Re: V359 Cen: definite SU UMa-type dwarf nova! Dear Colleagues, Roland Santallo (Southern Stars Observatory Tahiti) has just reported the result of time-series photometry of V359 Cen tonight. The light curve still clearly shows fully developed superhumps! The best period determined from the 2-night runs is 0.08136(8) d (=117 min). Further observations at different longitudes are also very strongly encouraged. The superhump profile is posted at: http://vsnet.kusastro.kyoto-u.ac.jp/pub/vsnet/DNe/V359_Cen/v359sh.gif Regards, Taichi Kato Roland Santallo VSNET Collaboration team
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