Generic predictions of LCDM hydrodynamical simulations on galaxy formation and evolution

Details Generic predictions of LCDM hydrodynamical simulations on galaxy formation and evolution Generic predictions of LCDM hydrodynamical simulations on galaxy formation and evolution

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...19711706n&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #117.06; Bulletin of the American Astronomical Society, Vol. 32, p.1603

Astronomy and Astrophysics

Astronomy

Scientific paper

I will discuss generic predictions of LCDM hydrodynamical simulations on galaxy formation and evolution, and compare them with observations. The simulations I use include a star formation recipe which allows us to investigate galaxy formation processes without ad-hoc assumptions of `bias' between galaxy and dark matter. The topics I will discuss include: the cosmic star formation history (Madau plot); the luminosity density of galaxies; the evolution of the galaxy mass function, luminosity function, and color; the cosmic Mach number statistic as a function of overdensity and galaxy age; and the number counts of galaxies in HDF.

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