Morphological decomposition of TNG50 galaxies: methodology and catalogue

Abstract

We present MORDOR (MORphological DecOmposeR, a new algorithm for structural decomposition of simulated galaxies based on stellar kinematics. The code measures the properties of up to five structural components (a thin/cold and a thick/warm disc, a classical and a secular bulge, and a spherical stellar halo), and determines the properties of a stellar bar (if present). A comparison with other algorithms presented in the literature yields overall good agreement, with MORDOR displaying a higher flexibility in correctly decomposing systems and identifying bars in crowded environments (e.g. with ongoing fly-bys, often observable in cosmological simulations). We use MORDOR to analyse galaxies in the TNG50 simulation and find the following: ($i$) the thick disc component undergoes the strongest evolution in the binding energy-circularity plane, as expected when disc galaxies decrease their turbulent-rotational support with cosmic time; ($ii$) smaller galaxies (with stellar mass, $10^9\lesssim M_{\ast }/{\mathrm{M}}_{\odot }\le 5\times 10^9$) undergo a major growth in their disc components after $z\sim 1$, whereas ($iii$) the most massive galaxies ($5\times 10^{10}<M_{\ast }/{\mathrm{M}}_{\odot }\le 5\times 10^{11}$) evolve toward more spheroidal dominated objects down to $z=0$ due to frequent gravitational interactions with satellites; ($iv$) the fraction of barred galaxies grows rapidly at high redshift and stabilizes below $z\sim 2$, except for the most massive galaxies that show a decrease in the bar occupation fraction at low redshift; ($v$) galaxies with $M_{\ast }\sim 10^{11}{\mathrm{M}}_{\odot }$ exhibit the highest relative occurrence of bars at $z=0$, in agreement with observational studies. We publicly release MORDOR and the morphological catalogue of TNG50 galaxies.

20 pages, 20 figures. Submitted to MNRAS. MORDOR is available at https://github.com/thanatom/mordor. The catalogue is available at www.tng-project.org/zana22

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