Galaxy evolution: Inhomogeneous halo collapse

Details Galaxy evolution: Inhomogeneous halo collapse Galaxy evolution: Inhomogeneous halo collapse

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.284..787m&link_type=abstract

Astrophysics and Space Science, v. 284, Issue 2, p. 787-790 (2003).

Astronomy and Astrophysics

Astrophysics

Galaxies: Evolution, Galaxies: Formation, Galaxies: Globular Clusters

Scientific paper

In an effort to study the halo globular clusters we perform a simulation of inhomogeneous halo collapse using a SPH/N-body code. We include dark matter particles, (cooling) gas, and stars. Supernova feedback is included as a heat source for the gas in the local environment of star forming regions. We find this model cannot reproduce the age distribution and spatial distribution of halo globular clusters.

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