[Open source - Linux] "Hubble in a bottle!" is visualization software for N-body simulations, which can be run in parallel using MPI for visualizing very large simulatio...
http://hubble.sourceforge.net
[open source - multiplatform] A guide to a tree code algorithm implementation, used for astronomical N-body simulations.
http://www.ifa.hawaii.edu/~barnes/software.html
Cloudy is an extensive, well-established, large-scale spectral synthesis code designed to simulate fully physical conditions within an astronomical plasma and then predict the emit...
http://www.nublado.org/
CMBEASY is a C++ code with GUI for calculation of CMB power spectra and other density fluctuation evolution data for a given cosmology.
http://www.cmbeasy.org/
COSMOMC calculates a fast Markov Chain Monte-Carlo exploration of cosmological parameter space for an input set of constraints.
http://cosmologist.info/cosmomc/
DUSTY calculates the emerging spectrum of radiation from some source viewed after processing by a dusty region. The original radiation is scattered, absorbed and reemitted by the d...
http://www.pa.uky.edu/~moshe/dusty/
Enzo is an adaptive mesh refinement (AMR), grid-based hybrid code (hydro + N-Body) which is designed to do simulations of cosmological structure formation.
http://cosmos.ucsd.edu/enzo/
EZ (Evolve ZAMS) Stellar Evolution tracks the evolution of new (Zero-Age Main Sequence) stars throughout the bulk of their lives (until an event which EZ does not model occurs, suc...
http://www.kitp.ucsb.edu/~paxton/EZ-intro.html
The FLASH code is a reacting hydrodynamics code with adaptive mesh refinement for general astrophysical hydrodynamics problems.
http://flash.uchicago.edu/
The Gadget-2 code is an SPH simulation code designed for cosmological simulations but can be used for a wide variety of astrophysical hydrodynamics simulations with self-gravity.
http://www.mpa-garching.mpg.de/gadget/
[open source - Unix] An extendible stellar dynamics toolbox; has various programs to create, integrate, analyze and visualize N-body and SPH-like systems. In addition there are var...
http://bima.astro.umd.edu/nemo/
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