Light variation of LX Persei between eclipses

Details Light variation of LX Persei between eclipses Light variation of LX Persei between eclipses

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..95..409i&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 95, no. 2, Sept. 1983, p. 409-416.

Astronomy and Astrophysics

Astrophysics

5

Eclipsing Binary Stars, Electrophotometry, Radiant Flux Density, Stellar Spectrophotometry, Light Curve, Orbital Elements, Periodic Variations, Spectral Energy Distribution

Scientific paper

Two-colour photoelectric observations of LX Per carried out at Ege University Observatory in 1981 and 1982 observing seasons are presented. The light curve of the system has a wave-like distortion which migrates towards the decreasing orbital phase. The period of the retrograde migration of the wave-like distortion has been determined as 475 days. The amplitude of the wave appears to change with time periodically.

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