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Photometric analysis of the eclipsing binary V1425 Cygni

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Abstract

Photoelectric B and V light curves of the eclipsing binary V1425 Cygni were analyzed by the method of Wilson-Devinney. The system was found to be a semi-detached binary where the secondary component (less massive and cooler) fills its Roche lobe.

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Authors and Affiliations

  1. Ege University Observatory, Bornova, Izmir, Turkey

    Ö. L. Deĝirmenci, Ö. Gülmen, C. Sezer, N. Güdür & A. Erdem

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  1. Ö. L. Deĝirmenci
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  2. Ö. Gülmen
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  3. C. Sezer
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  4. N. Güdür
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  5. A. Erdem
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Deĝirmenci, Ö.L., Gülmen, Ö., Sezer, C. et al. Photometric analysis of the eclipsing binary V1425 Cygni. Astrophys Space Sci 241, 327–332 (1996). https://doi.org/10.1007/BF00645233

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  • DOI: https://doi.org/10.1007/BF00645233

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