Identikit 2: An Algorithm for Reconstructing Galactic Collisions
Jan, 201114 pages
Published in:
- Mon.Not.Roy.Astron.Soc. 413 (2011) 2860
e-Print:
- 1101.5671 [astro-ph.CO]
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Abstract: (arXiv)
Using a combination of self-consistent and test-particle techniques, Identikit 1 provided a way to vary the initial geometry of a galactic collision and instantly visualize the outcome. Identikit 2 uses the same techniques to define a mapping from the current morphology and kinematics of a tidal encounter back to the initial conditions. By requiring that various regions along a tidal feature all originate from a single disc with a unique orientation, this mapping can be used to derive the initial collision geometry. In addition, Identikit 2 offers a robust way to measure how well a particular model reproduces the morphology and kinematics of a pair of interacting galaxies. A set of eight self-consistent simulations is used to demonstrate the algorithm's ability to search a ten-dimensional parameter space and find near-optimal matches; all eight systems are successfully reconstructed.Note:
- 14 pages, 8 figures. Accepted for publication in MNRAS. To get a copy with high-resolution figures, use the web interface, or download the Identikit software, visit http://www.ifa.hawaii.edu/faculty/barnes/research/identikit/
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