Halo and Galaxy Clustering in the Early Universe

Details Halo and Galaxy Clustering in the Early Universe Halo and Galaxy Clustering in the Early Universe

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..990..467r&link_type=abstract

FIRST STARS III: First Stars II Conference. AIP Conference Proceedings, Volume 990, pp. 467-469 (2008).

Computer Science

Dark Matter, Population Iii Stars, Galactic Halo, Star Formation, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies

Scientific paper

Using an array of dark matter simulations, we explore the clustering properties of high redshift halos, including those large enough to host stars or galaxies. The simulations resolve down to the ``mini-halo'' mass scale at redshifts as high as 30, thus encompassing the expected full mass range of halos capable of hosting luminous objects and sources of reionization. Results are compared with analytical expectations, and implications for reionization are discussed.

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