SS Bootis - A totally eclipsing binary of the RS CVn type

Details SS Bootis - A totally eclipsing binary of the RS CVn type SS Bootis - A totally eclipsing binary of the RS CVn type

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aj.....88.1257w&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 88, Aug. 1983, p. 1257-1263.

Astronomy and Astrophysics

Astronomy

9

Eclipsing Binary Stars, Stellar Spectrophotometry, Ephemerides, Light Curve

Scientific paper

Photoelectric photometry gathered for SS Bootis over the 1976-1981 period shows a distortion wave amplitude variation from 0.05 to 0.20 mag, with no apparent pattern. From the rectified light curve, a new time of midprimary eclipse was found to be 2444332.0335 + or - 0.0005 days. Solutions of the primary eclipse data, rectified for star spots as well as for ellipticity and reflection, are presented.

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