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M. Westover, L. Hernquist (Harvard-Smithsonian CfA), V. Springel (MPA)
We use cosmological SPH simulations to identify galaxy mergers at high redshift (z = 3-4). We compare the clustering properties of the mergers to those of Lyman break galaxies and Lyman alpha emitters and discuss the possibility of those objects being merger-driven starbursts. We also study the time evolution of the galaxy merger rate to redshift zero.
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Bulletin of the American Astronomical Society, 34, #4
© 2002. The American Astronomical Soceity.