Bulut, I.2025-01-272025-01-2720091384-1076https://doi.org/10.1016/j.newast.2009.02.007https://hdl.handle.net/20.500.12428/25532The apsidal motion analysis of the eccentric eclipsing binaries: V397 Cep, V493 Car and BW Aqr have been presented. The method described by Lacy (1992) [Lacy, C.H S.. 1992. AJ 104, 2213] has been used for the apsidal motion analysis. The apsidal motion periods have been found to be 174.2 +/- 1.4, 277.3 +/- 21.3 and 7195 +/- 174 years for V397 Cep, V493 Car and BW Aqr, respectively. (C) 2009 Elsevier B.V. All rights reserved.eninfo:eu-repo/semantics/closedAccessStars: binariesStars: binaries: eclipsingStars: individual: V397 Cep, V493 Car, BW AqrArticle14760460610.1016/j.newast.2009.02.007Q3WOS:0002665242000022-s2.0-67349101162Q2