Photometry of EF Pegasi during superoutburst
Publications of the Astronomical Society of the Pacific1993Vol. 105, pp. 579–579
Citations Over Time
Abstract
EF Pegasi was observed photometrically during a superoutburst in 1991 October. Superhumps seen during these observations were best fit with a period of 2h .09. This period is used to determine a likely orbital period of 2h .05 and a mass ratio (M2/M1) of 0.26. Distance estimates for EF Peg give values of 250 to 600 pc.
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