Abstract
We report on two fully self-consistent hydrodynamical simulations run, in the context of a ΛCDM cosmological model, with the DEVA code. Galaxy-like-objects of different morphologies form. The assembly patterns identified in these simulations give support to the ab initio scenario to explain morphological differentiation, even if violent events at lower z could also have played a role.
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DomÍnguez-Tenreiro, R., Serna, A., Sáiz, A. et al. Clues on the Hubble sequence formation from self-consistent hydrodynamical simulations. Astrophysics and Space Science 284, 397–400 (2003). https://doi.org/10.1023/A:1024011001092
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DOI: https://doi.org/10.1023/A:1024011001092