Apsidal motion elements of three eccentric eclipsing binaries: V397 Cep, V493 Car and BW Aqr


Bulut I.

NEW ASTRONOMY, vol.14, no.7, pp.604-606, 2009 (Journal Indexed in SCI) identifier identifier

  • Publication Type: Article / Article
  • Volume: 14 Issue: 7
  • Publication Date: 2009
  • Doi Number: 10.1016/j.newast.2009.02.007
  • Title of Journal : NEW ASTRONOMY
  • Page Numbers: pp.604-606

Abstract

The 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.