THE EFFECT OF CHEMICAL ABUNDANCE OSCILLATIONS ON THE PULSATIONAL PROPERTIES OF A 5 M-CIRCLE-DOT HYDROGEN-HELIUM STAR

UYANIKER B., KIRBIYIK H.

ASTROPHYSICS AND SPACE SCIENCE, cilt.192, sa.2, ss.275-289, 1992 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 192 Sayı: 2
  • Basım Tarihi: 1992
  • Doi Numarası: 10.1007/bf00684485
  • Dergi Adı: ASTROPHYSICS AND SPACE SCIENCE
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.275-289
  • Orta Doğu Teknik Üniversitesi Adresli: Hayır

Özet

A model of a first generation intermediate star of 5 M., with Z = 0 has been considered. The model is at an advanced stage of its evolution and has a double shell burning. It burns helium in the inner shell, and hydrogen, via CNO cycle, in the outer shell.