Revised photometric analysis of the eclipsing binary V 1073 Cygni

Sezer, C

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Publication date

January 1996

DOI

10.1007/BF00637805

Publisher

Springer Science and Business Media LLC

Journal

Astrophysics and Space Science

Abstract

WOS: A1996XL08400007Photoelectric light curves of the eclipsing binary V 1073 Cygni were analyzed with the Wilson-Devinney method and published previously. The spectral type of the primary component was given as A3 in the literature and our solutions were based to this spectral type. A recent spectroscopic investigation (Ahn et al., 1992) showed that V 1073 Cygni is an early F star and not an A3Vm star. In order to obtain accurate solutions in this situation, the light curves were reanalyzed by means of the Wilson-Devinney computer code

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Revised photometric analysis of the eclipsing binary V 1073 Cygni

Abstract

Extracted data

Revised photometric analysis of the eclipsing binary V 1073 Cygni

Abstract

Extracted data

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