High Resolution Coude Echelle Spectroscopy of IX Per


FİLİZ AK N., Eker Z., FİLİZ AK N., Kuecuek I.

15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, St Andrews, Scotland, 21 - 25 July 2008, vol.1094, pp.632-633 identifier identifier

  • Publication Type: Conference Paper / Full Text
  • Volume: 1094
  • Doi Number: 10.1063/1.3099193
  • City: St Andrews
  • Country: Scotland
  • Page Numbers: pp.632-633

Abstract

High resolution (R=45033) Coude - Echelle spectra of IX Per has been obtained at TUBITAK National Observatory (TUG) of Turkey. IX Per has been known to be a single lined (SBI) spectroscopic binary having chromospheric activity. However, analyzed spectra of IX Per by KOREL disentangling method indicated that the system is a double lined (SB2) spectroscopic binary. Weaker lines from the secondary arc discovered on the decomposed spectra. A preliminary orbit indicates that the mass ratio of the system is 0.64. The light contribution of the secondary is tip to 10% in investigated spectral region. Circular orbit is sufficient to explain radial velocity variations.