Thermal and Dynamical Properties of a Protostar and Its Contraction to the Stage of Quasi-Static Equilibrium

  • Hayashi C
  • Nakano T
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Abstract

… beginning of quasi-hydrostatic … quasi-hydrostatic equilibrium, and in a short period of about 10 3 years the star becomes wholly convective. The subsequent evolution is a quasi-static …

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Hayashi, C., & Nakano, T. (1965). Thermal and Dynamical Properties of a Protostar and Its Contraction to the Stage of Quasi-Static Equilibrium. Progress of Theoretical Physics, 34(5), 754–775. https://doi.org/10.1143/ptp.34.754

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