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Dear Taichi, WX Cen has been around 12.8CR in March 2003 and 13.2CR in April 2003. This from CBA monitoring. Assuming V-CR=0, the bright state seems to be continuing. Great input from ASAS though. Variable star observing will never be the same again in the South. I must also mention that I have discovered several fast variable stars in the fields that I monitored for CBA and VSNET. Composing deep field images and data mining are part of my pre-data-erase procedure for those large image files. ASAS has hinted at some useful ideas! Regards, Berto Monard Bronberg Observatory / CBA Pretoria >>> Taichi Kato <tkato@kusastro.kyoto-u.ac.jp> 05/01/03 10:35AM >>> WX Cen brightening? According to the ASAS-3 survey data, the V Sge/SSS type WX Cen may be brightening (currently around V=13.1). Probably worth observing. Regards, Taichi Kato -- This message has been scanned for viruses and dangerous content by MailScanner, and is believed to be clean. Mailscanner thanks transtec Computers for their support.
Return to the Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
