Galactic evolution. I - Single-zone models

Details Galactic evolution. I - Single-zone models Galactic evolution. I - Single-zone models

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...201..756t&link_type=abstract

Astrophysical Journal, vol. 201, Nov. 1, 1975, pt. 1, p. 756-772.

Physics

24

Astronomical Models, Galactic Evolution, Stellar Evolution, Abundance, Metallic Stars, Stellar Mass, Stellar Motions, Stellar Physics, White Dwarf Stars

Scientific paper

The two basic approaches of physical theory required to calculate the evolution of a galactic system are considered, taking into account stellar evolution theory and the dynamics of a gas-star system. Attention is given to intrinsic (stellar) physics, extrinsic (dynamical) physics, and computations concerning the fractionation of an initial mass of gas into stars. The characteristics of a 'standard' model and its variants are discussed along with the results obtained with the aid of these models.

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