An oscillating model suggestion for 63 Her


Kiziloglu N., Kirbiyik H., Civelek R.

ASTRONOMISCHE NACHRICHTEN, cilt.324, sa.3, ss.215-218, 2003 (SCI İndekslerine Giren Dergi) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 324 Konu: 3
  • Basım Tarihi: 2003
  • Doi Numarası: 10.1002/asna.200310082
  • Dergi Adı: ASTRONOMISCHE NACHRICHTEN
  • Sayfa Sayıları: ss.215-218

Özet

An attempt has been made towards explaining the observed frequencies in 63 Her. The evolution of rotating stars of 1.96, 1.98, 2.00, 2.05 and 2. 10 M-circle dot have been studied up to a point where stellar parameters match the observed luminosity and effective temperature of 63 Her. Radial and nonradial adiabatic oscillation frequencies were obtained in low harmonic degrees ( 1 = 0,1,2,3). One radial and three nonradial frequency values that match with the observed values were found for the model of mass 2.00 M-circle dot.