Assessing the influence of metallicity on fragmentation of proto-galactic gas

Details Assessing the influence of metallicity on fragmentation of proto-galactic gas Assessing the influence of metallicity on fragmentation of proto-galactic gas

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007hia....14..268j&link_type=abstract

Highlights of Astronomy, Volume 14, p. 268-268

Astronomy and Astrophysics

Astronomy

Stars: Formation, Methods: Numerical, Hydrodynamics, Early Universe

Scientific paper

In cold dark matter cosmological models, the first stars to form are
believed to do so within small protogalaxies. We study the influence of
low levels of metal enrichment on the cooling and collapse of ionized
gas in these protogalactic halos using three-dimensional, smoothed
particle hydrodynamics simulations.

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