Halos and Star Formation in the Dark Ages

Details Halos and Star Formation in the Dark Ages Halos and Star Formation in the Dark Ages

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...20715201r&link_type=abstract

American Astronomical Society Meeting 207, #152.01; Bulletin of the American Astronomical Society, Vol. 37, p.1411

Astronomy and Astrophysics

Astronomy

Scientific paper

We use high-resolution N-body simulations to compute the number of halos in the high redshift universe, and we compare the results with analytic predictions. We model gas cooling in these halos in order to calculate the number of halos capable of hosting stars and galaxies in the pre-reionized universe (the ``dark ages"). We discuss possibilities for observing these high redshift objects.

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