What is NEMO?

NEMO is an extendible Stellar Dynamics Toolbox. It has various programs to create, integrate, analyze and visualize N-body and SPH like systems. In addition there are various tools to operate on images, tables and orbits, including FITS files to export/import to/from other astronomical data reduction packages.

* Startup

If you add the following command to you .cshrc file:
        alias nemo 'source /local/rc/nemo.csh'
you can load NEMO into your environment by issuing the command
        nemo
each time when you have started a new shell (or opened a new window). To get the most out of NEMO make sure you understand:

* Examples

Here is the example that was discussed in class.

Conversion of an Ascii table output file:

Make sure the tabular output of your N-body integrator is a set of snapshots, where each snapshot is labeled with the time and the number of bodies in that snapshot, followed by all the particle positions and velocities, one on each line. Here is an example of 8 particles, at rest at the edges of a cube of size 1, at snapshot time 2.00:
    2.00  8
    0.0 0.0 0.0 0.0 0.0 0.0
    0.0 0.0 1.0 0.0 0.0 0.0
    0.0 1.0 0.0 0.0 0.0 0.0
    0.0 1.0 1.0 0.0 0.0 0.0
    1.0 0.0 0.0 0.0 0.0 0.0
    1.0 0.0 1.0 0.0 0.0 0.0
    1.0 1.0 0.0 0.0 0.0 0.0
    1.0 1.0 1.0 0.0 0.0 0.0
The following NEMO commands would convert and display this data:
    tabtos in=cube.tab out=cube.snap header=time,nbody block1=pos,vel
    snapshot in=cube.snap
or alternatively using a completely different package XGobi:
    snapprint cube.snap | xgobi
you can do some interactive 3D viewing (there are also programs for this in NEMO, e.g. snapxyz and xyzview)

* Documentation

* References


teuben@astro.umd.edu. 11-nov-97