Identikit 2: an algorithm for reconstructing galactic collisions

被引:17
作者
Barnes, Joshua E. [1 ]
机构
[1] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
关键词
methods: numerical; galaxies: interactions; galaxies: kinematics and dynamics; DARK-MATTER HALOS; ORBITAL PARAMETERS; TIDAL TAILS; GENETIC ALGORITHM; ROTATION CURVES; DISK GALAXIES; COLD; NGC-7252;
D O I
10.1111/j.1365-2966.2011.18358.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:2860 / 2872
页数:13
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