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, İskoçya, 21 - 25 Temmuz 2008, cilt.1094, ss.632-633 identifier

  • Cilt numarası: 1094
  • Basıldığı Şehir: St Andrews
  • Basıldığı Ülke: İskoçya
  • Sayfa Sayıları: ss.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.