Dynamical Modeling of Galaxy Mergers using Identikit
G. C. Privon, J. E. Barnes, A. S. Evans, J. E. Hibbard, M. S. Yun, J., M. Mazzarella, L. Armus, J. Surace

TL;DR
This paper models four galaxy mergers using the Identikit tool, combining rapid hybrid simulations with self-consistent models to reproduce observed features and infer merger stages, demonstrating the method's effectiveness.
Contribution
First application of Identikit to NGC 5257/8 and NGC 2623, validating its utility in constraining galaxy merger parameters with real data.
Findings
Models reproduce observed morphology and ext{H} ext{I} kinematics.
Estimated merger stages are 175-260 Myr after first passage.
Identikit effectively constrains merger parameters despite some mismatches.
Abstract
We present dynamical models of four interacting systems: NGC 5257/8, The Mice, the Antennae, and NGC 2623. The parameter space of the encounters are constrained using the Identikit model-matching and visualization tool. Identikit utilizes hybrid N-body and test particle simulations to enable rapid exploration of the parameter space of galaxy mergers. The Identikit-derived matches of these systems are reproduced with self-consistent collisionless simulations which show very similar results. The models generally reproduce the observed morphology and \HI\ kinematics of the tidal tails in these systems with reasonable properties inferred for the progenitor galaxies. The models presented here are the first to appear in the literature for NGC 5257/8 and NGC 2623, and The Mice and the Antennae are compared with previously published models. Based on the assumed mass model and our derived…
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Taxonomy
TopicsInnovation Diffusion and Forecasting
