Governato, Colpi and Maraschi 1994
The files k17c.snap.gz
contain the final merger remnants from runs k17c
and k17hp as described in
"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
x y z
vx vy vz
eps (and NOT the potential)