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PHOTOELECTRIC  PHOTOMETRY  OF  V491  LYRAE  AND  LM  PEGASI

 

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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

 

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.

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