On the Stellar Convective Zone and the Stellar Evolution

환성(桓星)의 대유층(對流層)과 그 진화(進化)

  • Hyun, Jong-June (Department of Astronomy, College of Natural Science, Seoul National University)
  • 현정준 (서울대학교 자연과학대학 천문학과)
  • Published : 1975.12.31

Abstract

Effect of the ratio of mixing length to the pressure scale-height ${\alpha}$=l/HP on the effective temperature has been investigated under some simplifying assumptions. The result is compared with that of the existing model calculations. The role of convection zone in the stellar evolution is briefly summarized.

Keywords