ROTATIONAL EVOLUTION OF THE SUN

KIZILOGLU N.

ASTROPHYSICS AND SPACE SCIENCE, cilt.192, sa.1, ss.83-89, 1992 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 192 Sayı: 1
  • Basım Tarihi: 1992
  • Doi Numarası: 10.1007/bf00653263
  • Dergi Adı: ASTROPHYSICS AND SPACE SCIENCE
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.83-89
  • Orta Doğu Teknik Üniversitesi Adresli: Hayır

Özet

The evolutionary behaviour of rotating solar models with different initial angular-momentum distributions has been investigated through the pre-Main-Sequence and Main-Sequence phases. The angular momentum was removed from the convective envelope of the solar models according to the Kawaler's model of magnetic stellar wind (Kawaler, 1988). The models show that (i) the surface rotational velocities of the solar mass stars are independent of initial angular momentum for ages greater than 10(8) years and (ii) it is not possible to explain the neutrino problem and the sufficient depletion of lithium in the Sun.