Abstract
UBV observations of the short-period eclipsing binary BW Eri are reported and analyzed. The photometric parameters are determined. BW Eri is a detached or semidetached system.
Similar content being viewed by others
References
Baade, D., Duerbeck, H. W., and Karimie, M. T.: 1979,Inf. Bull. Variable Stars, No. 1568.
Hoffmeister, C.: 1936,Astron. Nachr. 258, 39.
Kopal, Z.: 1959,Close Binary Systems, Chapman and Hall, London.
Lucy, L. B. and Wilson, R. E.: 1979,Astrophys. J. 231, 502.
Rucinski, S. M.: 1969,Acta Astron. 19, 125.
Schlesinger, F. and Barney, I.: 1943,Trans. Astron. Obs. Yale Univ. 13, pt. 2.
Schmidt-Kaler, Th.: 1982,Landolt-Börnstein N. S. VI/2b,, 1, Springer, Berlin.
Solov'yov, A. V.: 1954,Astron. Tsirk. 151, 25.
Yamasaki, A.: 1981,Astrophys. Space Sci. 77, 75.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Baade, D., Duerbeck, H.W., Karimie, M.T. et al. A photometric study of the short-period eclipsing binary BW Eridani. Astrophys Space Sci 88, 197–204 (1982). https://doi.org/10.1007/BF00649000
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00649000