Revised photometric elements of three semi-detached binary systems

Details Revised photometric elements of three semi-detached binary systems Revised photometric elements of three semi-detached binary systems

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..82..189m&link_type=abstract

Astrophysics and Space Science, vol. 82, no. 1, Feb. 1982, p. 189-198. Research supported by the Consiglio Nazionale delle Rice

Astronomy and Astrophysics

Astrophysics

3

Eclipsing Binary Stars, Light Curve, Stellar Models, Stellar Spectrophotometry, A Stars, Astronomical Photometry, Mass To Light Ratios, Roche Limit, Stellar Evolution, Stellar Mass

Scientific paper

It is found through analysis of the V and B light curves of the UZ Cyg, VW Cyg and AQ Peg Algol-type eclipsing binaries by the Wilson and Devinney (1971) model that all are semi-attached systems, with A-type primary components and K-type evolved secondary which fill the corresponding lobe. Only VW Cyg may alternatively be considered an sd-d system. The computing procedures employed have been described by Maceroni et al, (1981) and Milano et al (1981b).

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