Substructure in Galaxy Clusters: Discriminating Between Mergers and Accretions

Details Substructure in Galaxy Clusters: Discriminating Between Mergers and Accretions Substructure in Galaxy Clusters: Discriminating Between Mergers and Accretions

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apl%26c..36..133g&link_type=abstract

Astrophysics Letters and Communications, 1995, Vol. 31, p. 45

Astronomy and Astrophysics

Astrophysics

Galaxies, Clusters, Large Scale Structure Formation

Scientific paper

The origin of small-scale substructure is traced back to merger remnants
by comparing the output of N-body simulations of clusters mergers with
the results of a previously analyzed sample of real clusters.

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