A family of potential-density pairs for galactic bars
arXiv:2210.14853 · doi:10.1093/mnras/stac3124
Abstract
We present a family of analytical potential-density pairs for barred discs, which can be combined to describe galactic bars in a realistic way, including boxy/peanut components. We illustrate this with two reasonable compound models. Computer code for the evaluation of potential, forces, density, and projected density is freely provided.
arXiv comment10 pages, accepted for publication at MNRAS
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