At its core NEMO defines a series of objects (SnapShot, Orbit, Image) and associated header files and libraries to operate on them, and these mirror the stored data in a portable binary-named and type-tagged XML-like format dubbed structured file.
The program tsf in NEMO will show the contents of such a file in a human readable way.
For example, would create a 1000 particle Plummer sphere, scale the velocities down to below virial equilibrium, integrate this for 10 virial times to see it collapse, and take the particle distribution of the last snapshot and turn that into a FITS file to view in another astronomical analysis package.
NEMO was conceived and written by Josh Barnes, Piet Hut and Peter Teuben in 1986, at the Institute for Advanced Study, prompted by the wish to have a toolkit built around the just developed Barnes–Hut simulation.
[1] NEMO was presented at the 1994 Astronomical Data Analysis Software and Systems (ADASS) conference held in Baltimore, MD.