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.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 2years
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UNVERDICTED 2representative citing papers
Deep g,r,i photometry of IC 5332 shows redder color gradients in the outskirts and faint stellar streams, supporting ongoing stellar mass assembly via accretion.
citing papers explorer
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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.
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VST-SMASH: VST Survey of Mass Assembly and Structural Hierarchy I. Survey presentation and deep photometry of IC 5332: tracing the mass assembly in the challenging faintest-end regime
Deep g,r,i photometry of IC 5332 shows redder color gradients in the outskirts and faint stellar streams, supporting ongoing stellar mass assembly via accretion.