Testing an SPH code following the evolution of a CDM protogalaxy.

Details Testing an SPH code following the evolution of a CDM protogalaxy. Testing an SPH code following the evolution of a CDM protogalaxy.

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apl%26c..36..339v&link_type=abstract

Astrophysical Letters and Communications, Vol. 36, Nos. 1 - 6, p. 339 - 344

Astronomy and Astrophysics

Astrophysics

Galaxy Formation: Numerical Simulations, Galaxy Clustering: Numerical Simulations

Scientific paper

The reliability of the SPH code is tested in order to follow the
dynamical evolution of galaxy clusters.

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