Abstract
Photoelectric observations of the eclipsing binary GO Cyg have been carried out inB andV colours at the Ege University Observatory. The corresponding light curves were analyzed by the method of Wilson-Devinney. The system was found to be a reverse Algol semi-detached binary. The absolute elements of the system are also deduced.
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Cester, B., Giuricin, G., Mardirossian, F., and Mezzetti, M.: 1979,Acta Astron. 29, 433.
Grygar, J., Cooper, M. L., and Jurkevich, I.: 1972,Bull. Astron. Inst. Czech. 23, 147.
Hall, D. S. and Louth, H.: 1990,J. Astrophys. Astron. 11, 271.
Kukarkin, B. W.: 1929,N. N. V. S. 2, 26.
Kukarkin, B. W.: 1932,N. N. V. S. 4, 19.
Leung, K. C.: 1988, in K. C. Leung (ed.),Critical Observations versus Physical Models for Close Binary Systems, Gordon and Breach Science Publishers, New York, p. 93.
Liau, S. P.: 1935,Publ. Obs. Lyon, Ser.I, 1, Fasc. 13.
Lucy, L. B.: 1967,Z. Astrophys. 65, 89.
Mannino, G.: 1963,Publ. Univ. Bologna, Vol. 8, No. 15.
Ovenden, M. W.: 1954,Monthly Notices Roy. Astron. Soc. 114, 569.
Pearce, J. A.: 1933,J. R. Astron. Soc. Can. 27, 62.
Pierce, N. L.: 1939,Astron. J. 48, 113.
Popper, D. M.: 1957,Astrophys. J. Suppl. 3, 107.
Popper, D. M.: 1980,Ann. Rev. Astron. Astrophys. 18, 115.
Rovithis, P., Rovithis-Livaniou, H., and Niarchos, P. G.: 1990,Astron. Astrophys. Suppl. Ser. 83, 41.
Schneller, H.: 1928,Astron. Nachr. 235, 85.
Sezer, C., Gülmen, Ö., and Güdür, N.: 1985,Inf. Bull. Var. Stars, No. 2743.
Szczyrbak, S.: 1932,S. A. C. 10, 44.
von Zeipel, H.: 1924,Monthly Notices Roy. Astron. Soc. 84, 665.
Wilson, R. E. and Devinney, E. J.: 1971,Astrophys. J. 166, 605.
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Sezer, C., Gülmen, Ö. & Güdür, N. Photometry and analysis of the eclipsing variable GO Cygni. Astrophys Space Sci 203, 121–133 (1993). https://doi.org/10.1007/BF00659416
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DOI: https://doi.org/10.1007/BF00659416