Starspots on the primary components of V523 Cassiopeiae and CC Comae Berenices

Details Starspots on the primary components of V523 Cassiopeiae and CC Comae Berenices Starspots on the primary components of V523 Cassiopeiae and CC Comae Berenices

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..101z&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Feb. 1985, p. 101-106) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Jan.-Feb

Astronomy and Astrophysics

Astronomy

3

Astronomical Photometry, Binary Stars, Light Curve, Starspots, Cassiopeia Constellation, Stellar Oscillations

Scientific paper

Broadband photometric observations of the W UMa systems V523 Cas and CC Com have been carried out using the 60-cm reflector telescope of the Shternberg Astronomical Institute Southern Station, together with the 48-cm reflector of the Shternberg High-Altitude Station at Alma Ata, USSR. Mean B-V colors measured for V523 Cas are given in addition to the photometric orbital elements derived from spot-free light curves. It is shown that the long-term fluctuations in the light curves and B-V colors of V523 and CC Com are due to cool starspots on the surface of the primary component.

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