 Web Results |
| | The Art of Computational Science
An online `socratic book' pedagogically describing the building of a N-body simulation code for stellar systems. Software (in Ruby) is included.
http://www.artcompsci.org/ | | | Barnes & Hut Treecode Algorithm
multiplatform] A guide to a tree code algorithm implementation, used for astronomical N-body simulations.
http://www.ifa.hawaii.edu/~barnes/software.html | | | CAPGADGET
multiplatform] Visualization package to capture and display Gadget N-body simulations.
http://www.geocities.com/capgadget/ | | | Cloudy & Associates
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 emitted spectrum. The web page contains links to papers published with cloudy, the most recent version of the software itself, and a discussion board.
http://www.nublado.org/ | | | DUSTY -- Radiation transfer through dust
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 dust, and the emerging processed spectrum often provides the only available information about the embedded object. DUSTY can handle both planar and centrally-heated spherical density distributions. The number of independent input model parameters is minimized by fully implementing the scaling properties of the radiative transfer problem, and the spatial temperature profile is found from radiative equilibrium at every point in the dusty region. DUSTY has built in optical properties for the most common types of astronomical dust and comes with a library for many other grains.
http://www.pa.uky.edu/~moshe/dusty/ | | | Enzo
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 Stellar Evolution
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, such as a Helium Flash or core crystallization). The code is clean and well documented. Links include a web interface to the code.
http://www.kitp.ucsb.edu/~paxton/EZ-intro.html |
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