Photometry of EF Pegasi during superoutburst

Details Photometry of EF Pegasi during superoutburst Photometry of EF Pegasi during superoutburst

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105..579h&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 688, p. 579-585.

Astronomy and Astrophysics

Astronomy

20

Cataclysmic Variables, Orbital Elements, Stellar Flares, Stellar Spectrophotometry, Charge Coupled Devices, Stellar Mass Ejection

Scientific paper

EF Pegasi was observed photometrically during a superoutburst in October
1991. Superhumps seen during these observations were best fit with a
period of 2.09 h. This period is used to determine a likely orbital
period of 2.05 h and a mass ratio (M2/MI) of 0.26. Distance estimates
for EF Peg give values of 250 to 600 pc.

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