The Photometric Periods of the Nova-Like Cataclysmic Variable LQ Pegasi   (PG 2133+115)
  We present a time-resolved differential photometric study and time series analysis of the nova-like cataclysmic variable star LQ Peg. We discover three periodicities in the photometry, one with a period of 3.42 +/- 0.03 hours, and another with a period of 56.8 +/- 0.01 hours. We interpret these to be the apsidal superhump and precessional periods of the accretion disk, respectively, and predict that the orbital period of LQ Peg is 3.22 +/- 0.03 hours. The third periodicity, with a period of 41.3 +/- 0.01 hours, we interpret to be the nodal precessional period of the accretion disk. We also report a flare that lasted four minutes and had an energy in visible light of (1.2 +/- 0.3) x 10^36 ergs, or 10^4-5 times more energetic than the largest solar flares, comparable to the most energetic visible-light stellar flares known. We calculate the absolute magnitude of LQ Peg to be M_J = 4.78 +/- 0.54, and its distance to be 800 +/- 200 pc. 
Gerald D. Rude II and F. A. Ringwald
astro-ph.SR