The article we published
earlier on this star (Baldwin et al. 1976)
requires major revision and correction. Following our announcement of the extraordinarily
large change of period in this eclipsing binary we looked forward to the
arrival of the next observing season and collection of additional visual data
for further refinement oftheperiod. However, when the first minima of the
season were obtained they failed to confirm the new ephemeris. Minima continued
to occur more than six hours early as compared to elements by Kukarkin et
al. (1976)