Revised Photometric Analysis of the Eclipsing Binary V 1073 Cygni

Details Revised Photometric Analysis of the Eclipsing Binary V 1073 Cygni Revised Photometric Analysis of the Eclipsing Binary V 1073 Cygni

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.245...89s&link_type=abstract

Astrophysics and Space Science, Volume 245, Issue 1, pp.89-96

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

Photoelectric 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 (Ahnet al., 1992) showed that V 1073 Cygni is an early F star and not an A3 Vm 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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