A new series of observations of the small amplitude variables 3 Hya, 49 Cnc, and BX Boo similar to those of this paper in a few years should be able to improve all the periods. Some of the scatter might be reduced by making many observations in a semi-continuous mode during the course of only a few nights now that the periods are sufficiently well known for that purpose.
Acknowledgements
This work was supported in part by NSF grant AST-9528506 to The Citadel and in part by grants from The Citadel Development Foundation. I appreciate the continuing efforts of Louis J. Boyd and Robert J. Dukes, Jr., to keep the FCAPT operating properly.