Discs no more: the morphology of low-mass simulated galaxies in FIREbox.

Mon Not R Astron Soc · 2025 · PMC12680306 · PMID 41356272

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a clear trendno p-value reported

1 highlights a clear trend predicted in the morphology of simulated galaxies: while discs are frequent and dominant for MW-like galaxies ( \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{upgreek} \usepackage{mathrsfs} \setlengt

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