The V and B light curves of three Algol-type eclipsing binaries (UZ Cyg, VW Cyg, AQ Peg), observed by Amman et al. (1979), have been analysed using the Wilson and Devinney (1971) model. We find that all of them are semi-detached systems, with A-type primary components and K-type evolved secondary which fill the corresponding lobe, although VW Cyg should perhaps be considered as an sd-d system.
REVISED PHOTOMETRIC ELEMENTS OF THREE SEMI-DETACHED BINARY SYSTEMS / Milano, L.; Russo, G.; Marcozzi, S.; D'Orsi, A.. - In: ASTROPHYSICS AND SPACE SCIENCE. - ISSN 0004-640X. - 82:(1982), pp. 189-198.
REVISED PHOTOMETRIC ELEMENTS OF THREE SEMI-DETACHED BINARY SYSTEMS
L. MILANOMembro del Collaboration Group
;G. RUSSO
Membro del Collaboration Group
;
1982
Abstract
The V and B light curves of three Algol-type eclipsing binaries (UZ Cyg, VW Cyg, AQ Peg), observed by Amman et al. (1979), have been analysed using the Wilson and Devinney (1971) model. We find that all of them are semi-detached systems, with A-type primary components and K-type evolved secondary which fill the corresponding lobe, although VW Cyg should perhaps be considered as an sd-d system.File in questo prodotto:
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