Photoelectric Photometry of V491 Lyrae and LM Pegasi

Volume 29 number 2 (2001)

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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

Abstract

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.