We report the results of an analysis of the hierarchical properties of
the cluster of galaxies Abell II9. Observational data from the ESO Ne
arby Abell Cluster Survey (ENACS) are used, complemented by data from
previous studies, while the analysis is performed with the S-tree meth
od. The main physical system and three subgroups with truncated Gaussi
an velocity distributions are identified; we call these subgroups 'gal
axy associations'. The mass centre of the core of the main system is s
hown to coincide with the X-ray centre of the cluster. An alignment of
the mass centres of the three galaxy associations is also shown.