Photometric Study of the Light Curve of the Early Type Binary V1898 Cyg

Details Photometric Study of the Light Curve of the Early Type Binary V1898 Cyg Photometric Study of the Light Curve of the Early Type Binary V1898 Cyg

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007oejv...77....1a&link_type=abstract

Open European Journal on Variable Stars, vol. 0077, Issue 1, p.1

Computer Science

1

Scientific paper

The photoelectrical (BV)lightcurve of the eclipsing binary V1898 Cyg obtained by Dallaporta & Munari (2006) are here analyzed. The Wilson-Devinney Differential Correction program was used in the analysis and the results shows that the star is a semi-detached system with the secondary component that accurately fills its Roche lobe. The best fit was obtained at photometric mass ratio q = 0.3018 and inclination i = 70°

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