Polar-ring galaxies in the Illustris TNG50 simulation
Daniil V. Smirnov, Aleksandr V. Mosenkov, Vladimir P. Reshetnikov

TL;DR
This study uses the TNG50 simulation to identify and analyze the formation of polar-ring galaxies, revealing their origins through interactions and their impact on galaxy activity.
Contribution
First simulation-based analysis of PRGs in TNG50, identifying formation paths and their effects on galaxy properties.
Findings
Six stellar polar rings identified in TNG50.
Polar structures form via gas accretion or satellite disruption.
Ring inclination increases over billions of years.
Abstract
Polar-ring galaxies (PRGs) are an outstanding example of galaxies with misaligned kinematics where a typically red central galaxy is surrounded by a large-scale ring or disk of stars, gas and dust oriented almost perpendicular to the main body. It is believed that polar structures are formed in a secondary event after the assembly of a central galaxy, but due to their scarcity, their formation paths are not well constrained yet. We present a study of PRGs from TNG50 cosmological simulations, focusing on the origin of their polar structures. Based on the synthetic images and baryonic mass distribution, we found 6 galaxies with stellar polar rings. Using Supplementary Data Catalogues and available particle data, we confirm that the selected galaxies are direct analogs of real PRGs. In our sample, the polar structures are a result of the close interaction between the host galaxy and its…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
