Governato, Colpi and Maraschi 1994

The files k17c.snap.gz and k17hp.snap.gz contain the final merger remnants from runs k17c and k17hp as described in their paper "The fate of central black holes in merging galaxies" (MNRAS, in press) They are simple examples of an oblate rotator, partially rotation supported and a prolate system with mainly radial orbits. Models and initial conditions were generated with NEMO. The data format is the "205 format" (see also atos(1NEMO) ):

nbodies 
ndim
time
masses
x y z
vx vy vz
eps (and NOT the potential)