At z=1, disk galaxies exhibit U-shaped stellar age profiles with turnover at the edge, indicating inside-out growth with approximately 300% mass increase in outer regions since z=0.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Phylogenetic trees from stellar chemical abundances in a simulated disc galaxy reveal distinct structures in inner versus outer regions, indicating rapid early enrichment inside and smoother gradients outside.
citing papers explorer
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Witnessing the rapid growth of disk galaxies over cosmic time using JWST and HST
At z=1, disk galaxies exhibit U-shaped stellar age profiles with turnover at the edge, indicating inside-out growth with approximately 300% mass increase in outer regions since z=0.
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Reconstructing chemical enrichment pathways in disc galaxies: A phylogenetic approach
Phylogenetic trees from stellar chemical abundances in a simulated disc galaxy reveal distinct structures in inner versus outer regions, indicating rapid early enrichment inside and smoother gradients outside.