This is your cheat sheet for those running the TVO demo  (4-jan 11pm)
-------------------------------------------------------


0) check the timestamp at the top; URLs listed below may change slightly

1) point the browser to:    http://bima.astro.umd.edu/nemo/tvo/nvodemo2004
   or on peter's laptop:    http://localhost/www/nvodemo2004

   they both should work the same, but currently can each only run one demo 
   at a time!!   We don't save old data yet.

2) the main CMD comparison demo will be under the link "RUNIT" just 
   the picture of M3. 

   - select a cluster (the default is M30)
     no need to change the distance from the default, unless you want to play with it.

   - select a model (AMNH run3 is working ok, though the default button
	             may not seem to work upon first entry)

   - select a simulation time in MYr; 12000 Myr is ok.

   - The open cluster works very poorly with the amnh3 data, but try the amnh3 instead.


3) other things that can be shown:

   -  partiview animation of a N=10,000 cluster in space and time.
      Consumes about 350MB memory.
      On peter's laptop use a shell with starlab enabled:

            starlab
            cd tvo/www/grape/run2
            data2.cf
            
      loading can easily take 1-2 minutes, depending on what needs to be cleared
      from memory.


   -  a few quick links to manybody.org web demonstrations are also available. These
      are the result of the MODEST effort (dynamics+stellar evolution). In particular
      the 'binary evolution' and 'simple N-body integration' (with animations) are
      very visual and quick.




AMNH/Hurley (Aarseth's NBODY4 code on grape)

  run2	    N = 27k, 50% binaries, Z = 0.02
	    -> rich open cluster dead at ~6 Gyr

  run3      N = 100k, 0% binaries, Z = 0.001
	    -> small globular with 40k left at 12 Gyr