Photoelectric Photometry of V491 Lyrae and LM Pegasi

Details Photoelectric Photometry of V491 Lyrae and LM Pegasi Photoelectric Photometry of V491 Lyrae and LM Pegasi

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001javso..29...96k&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 29, no. 2, p.96

Physics

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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