High Resolution Coude Echelle Spectroscopy of IX Per

Ak N. , Eker Z., AK H. , 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

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


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.