Photoelectric observations and the wave minimum of RS CVn

Details Photoelectric observations and the wave minimum of RS CVn Photoelectric observations and the wave minimum of RS CVn

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.137...63s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 137, no. 1, Oct. 1987, p. 63-72.

Astronomy and Astrophysics

Astrophysics

Eclipsing Binary Stars, Electrophotometry, Stellar Spectrophotometry, Ubv Spectra, Wave Propagation, Light Curve, Stellar Color

Scientific paper

B, V observations of the eclipsing binary RS CVn have been presented. A dip around 0p.1 appears to be a wave minimum which fits well in the 'wave minimum phase-time' relation, but deviates from the 'wave amplitude-time' relation, derived for RS CVn. Either, the 'wave amplitude-time' relation requires a modification or the amplitude of the wave minimum appears masked by the intrinsic variability of one of the components or by the Sun-spot activity of the system. The colour exhibits variation. The secondary component appears active.

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