Photoelectric photometry of eclipsing binary V375 Cassiopeiae

Details Photoelectric photometry of eclipsing binary V375 Cassiopeiae Photoelectric photometry of eclipsing binary V375 Cassiopeiae

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986acaps...6..185z&link_type=abstract

(Acta Astrophysica Sinica, vol. 6, 1986, p. 185-192) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 10, Dec. 1986, p.

Astronomy and Astrophysics

Astrophysics

Eclipsing Binary Stars, Electrophotometry, Light Curve, Stellar Spectrophotometry, Roche Limit, Stellar Evolution, Stellar Mass

Scientific paper

Some 604 photoelectric BV observations of the eclipsing binary V375 Cas were obtained at Beijing Observatory from August to November 1982. The photometric solution was carried out using the Wilson-Devinney program for the BV light curves. The system is found to be a semi-detached binary in which the less massive component fills its Roche lobe and the more massive component nearly does so. It is very similar to RZ Dra. This very interesting system is important for the understanding of the evolution of close binaries.

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