Merger and Ring Galaxy Formation Rates at z<2
Mar, 2008Citations per year
Abstract: (arXiv)
We compare the observed merger rate of galaxies over cosmic time and the frequency of collisional ring galaxies (CRGs), with analytic models and halo merger and collision rates from a large cosmological simulation. In the Lambda cold dark matter (LCDM) model we find that the cosmic {\it merger fraction} does not evolve strongly between 0.2References(56)
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