Early-type galaxies at low Z from self-consistent hydrodynamical simulations

Details Early-type galaxies at low Z from self-consistent hydrodynamical simulations Early-type galaxies at low Z from self-consistent hydrodynamical simulations

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.284..411s&link_type=abstract

Astrophysics and Space Science, v. 284, Issue 2, p. 411-414 (2003).

Astronomy and Astrophysics

Astrophysics

4

Galaxies: Early-Type, Methods: Numerical

Scientific paper

We present results of an analysis of the properties of spheroid-like
galaxies that form in hydrodynamical, self-consistent cosmological
simulations run with the DEVA code. We find that the structural,
dynamical and X-ray properties, as well as their correlations, are
compatible with observations of early-type galaxies at low z.

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