Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.225p..21b&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 225, March 15, 1987, p. 21P-27P.
Astronomy and Astrophysics
Astronomy
13
Anisotropy, Galactic Evolution, Metallicity, Radial Velocity, Star Formation, Stellar Mass Ejection, Velocity Distribution
Scientific paper
Two-dimensional calculations of galaxy formation are presented. Gas and stars are taken into account as two distinct components interacting by star formation and stellar mass loss. While the gas is described by means of the Eulerian equation, the authors allow for an anisotropic velocity distribution among the stars by applying the collisionless Boltzmann equation. In their first model the authors succeed in developing totally different stellar populations forming a halo and a disc.
Burkert Andreas
Hensler Gerhard
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