Identikit 2: an algorithm for reconstructing galactic collisions
Abstract
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.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- June 2011
- DOI:
- 10.1111/j.1365-2966.2011.18358.x
- arXiv:
- arXiv:1101.5671
- Bibcode:
- 2011MNRAS.413.2860B
- Keywords:
-
- methods: numerical;
- galaxies: interactions;
- galaxies: kinematics and dynamics;
- Astrophysics - Cosmology and Nongalactic Astrophysics
- E-Print:
- 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/