Identikit is a numerical method, combining test-particle and self-consistent techniques, which allows a rapid exploration of the parameter space of galactic encounters. It can be used to find the parameters required to reproduce the observed morphology and kinematics of interacting disk galaxies.
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| Identikit model (points) matching a self-consistent N-body simulation of a galactic collision (grey scale). Each panel shows a different projection: top left shows sky-plane (X,Y), top right shows velocity-position (V, Y); bottom left shows position-velocity (X, V), bottom right shows (X, Z). |
— Paper describing the Identikit system and a blind test of its abilities. To appear in The Astronomical Journal, February 2009.
— Web interface to Identikit allows the user to select encounter and viewing parameters, and see the results instantaneously.
— Random merger simulations from the Identikit 1 paper; click on individual systems to see matches.
— Summary of the parameters needed to define an encounter between disk galaxies.
— Source code and key makefiles for Identikit. Requires Zeno software environment.
— Talk given at Academia Sinica Institute of Astronomy and Astrophysics, June 4, 2008.
— John Hibbard's page describing an earlier version.
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Joshua E. Barnes
(barnes at ifa.hawaii.edu)
Updated:
29 November 2008
http://www.ifa.hawaii.edu/~barnes/research/identikit/index.html |
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