Whitin Observatory, Wellesley College, Wellesley, MA 02181
observed water maser emission i R Ceti at 22 GHz at the Haystack Observatory
from January 23, 1985, to September 28, 1988. We have compared the water maser
data to visual data compiled by the AAVSO. The intensity of the water maser
emission varies in correlation with the visual light curve but with a phase lag
of 0.25. The intensity of the water emission varies from cycle to cycle.