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Daniel H. Kaiser

2631 Washington Street

Columbus, IN 47201


David B. Williams

P. O. Box 58

Whitestown, IN 46075


John E. Isles

11105 Tremont Lane

Plymouth, MI 48170


Received December 1, 2000




Photoelectric photometry of V491 Lyrae and LM Pegasi indicates that these stars are small-amplitude red semiregular variable stars. Observations of V491 Lyr ranged from 8.2-8.9 V with a period of 66.3 days. LM Peg varied from 9.0-9.5 V with a probable period of 68.6 days, although a denser time series of observations is needed to confirm this value.

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