High Redshift Galaxy Mergers in SPH Simulations

Details High Redshift Galaxy Mergers in SPH Simulations High Redshift Galaxy Mergers in SPH Simulations

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.5110w&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #51.10; Bulletin of the American Astronomical Society, Vol. 34, p.1191

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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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