Photoelectric Photometry of V491 Lyrae and LM Pegasi
Volume 29 number 2 (2001)
- 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.