Early pre-main sequence evolution of low mass stars

Kucuk I., Kiziloglu N., Civelek R.

ASTROPHYSICS AND SPACE SCIENCE, cilt.259, sa.3, ss.279-284, 1998 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 259 Sayı: 3
  • Basım Tarihi: 1998
  • Doi Numarası: 10.1023/a:1001522620068
  • Dergi Adı: ASTROPHYSICS AND SPACE SCIENCE
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.279-284
  • Orta Doğu Teknik Üniversitesi Adresli: Hayır

Özet

Evolution of the gravitational contraction phase of stars having masses 0.3 < M/M. < 1.5 were studied along with deuterium burning. The equation of state developed by Mihalas et al. (1988) and OPAL opacity tables were used in our investigation. The theoretical time Lines were compared with observations.