Clues on the Hubble sequence formation from self-consistent hydrodynamical simulations

Details Clues on the Hubble sequence formation from self-consistent hydrodynamical simulations Clues on the Hubble sequence formation from self-consistent hydrodynamical simulations

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.284..397d&link_type=abstract

Astrophysics and Space Science, v. 284, Issue 2, p. 397-400 (2003).

Astronomy and Astrophysics

Astrophysics

1

Galaxy: Formation, Evolution

Scientific paper

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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