Photoelectric Photometry of V491 Lyrae and LM Pegasi

Physics

Scientific paper

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V491 Lyrae, Lm Pegasi, Variable Stars, Photoelectric Photometry

Scientific paper

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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