Recent observations of the Coma cluster of galaxies in its central reg
ion have provided approximately 250 new redshifts - allowing a good me
mbership criterion to be established for brighter galaxies - and magni
tudes for 8000 objects in the same region derived from photometric dat
a complete up to V-26.5=22.5. A thorough structural study of the galax
y distribution of the cluster galaxies, jointly with an X-ray wavelet
analysis, and with a kinematical analysis of the velocity distribution
allows us to uncover a primary body of the cluster, with evidence for
a velocity gradient.