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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.
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