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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3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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UNVERDICTED 3representative citing papers
Uncertainties in stellar evolution and IMF lead to stellar mass errors of ~0.3 dex at z~0 and ~0.6 dex at z~2, plus ~0.4 mag uncertainty in K-band luminosity evolution per unit redshift.
A simple dry merger model based on infall formalism and Virial Theorem reproduces key features of galaxy scale relations including slopes, scatters, curvatures, and exclusion zones.
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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The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
Uncertainties in stellar evolution and IMF lead to stellar mass errors of ~0.3 dex at z~0 and ~0.6 dex at z~2, plus ~0.4 mag uncertainty in K-band luminosity evolution per unit redshift.
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A simple yet effective model of galaxy mergers
A simple dry merger model based on infall formalism and Virial Theorem reproduces key features of galaxy scale relations including slopes, scatters, curvatures, and exclusion zones.