Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.105...23t&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 105, no. 1, Oct. 1984, p. 23-31.
Astronomy and Astrophysics
Astrophysics
13
Astronomical Photometry, Eclipsing Binary Stars, Electrophotometry, Least Squares Method, Light Curve
Scientific paper
The RS CVn-type eclipsing binary SZ Psc was observed in two colours B and V, in 1981. The rate of change of the period was calculated using two different least-squares procedures. The amplitudes of the light variations at outside eclipses are 0m.181 and 0m.213 in B and V colours, respectively. The light curves of the system have been solved using a new approximation. The radius of the cooler component is only 82% of its Roche-radius and the system is detached.
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