A light-curve distortion-wave analysis of eight RS Canum Venaticorum systems

Details A light-curve distortion-wave analysis of eight RS Canum Venaticorum systems A light-curve distortion-wave analysis of eight RS Canum Venaticorum systems

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986aj.....91..132c&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 91, Jan. 1986, p. 132-138.

Astronomy and Astrophysics

Astronomy

12

Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Ubv Spectra, Distortion, Ephemerides, Fourier Transformation

Scientific paper

A program of differential U,B,V photometry of 14 RS CVn systems carried out at Rosemary Hill Observatory in 1978 - 1981 is described, and an analysis of the light curves for the characteristic distortion wave for eight of the systems is presented. The V light curves of the systems are shown. Significant waves were observed in RS CVn, RZ Eri, and RW UMa. No significant waves were found in UX Com, GK Hya, AR Lac, LX Per, or TY Pyx. Unusual light curve distortions were observed in UX Com and AR Lac.

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