You can see from the BAAVSS plot and also from the AAVSO plot of 1843-1972: http://vsnet.aavso.org/images/HISTRCRB.GIF that the typical RCB lightcurve hits bottom at ~8 mag below max. The lightcurve actually shows a flat bottom that it can't go below. At this point, we are seeing no direct light from the star and only scattered light from around the star. Other RCB stars show similar behaviour. Geoff Clayton
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