Chemically decoupled massive galaxies in IllustrisTNG dominate the high end of a present-day habitability proxy by over an order of magnitude due to a trade-off between suppressed planet formation and reduced sterilizing events.
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Green Pea and Blueberry galaxies live in isolated low-density environments with the lowest neighbor counts among compared galaxy populations.
Green valley galaxies live preferentially in the outskirts of galaxy clusters as satellites, consistent with environmental quenching processes.
Simulations show dense environments suppress dwarf satellite abundance relative to voids, with environment as the main driver over host stellar mass and morphology.
Stellar halos act as transition regions between bright central galaxies and intracluster light, with strong mass correlations, similar colors that redden over time, and a shrinking metallicity gap from 0.4 dex at z=2 to 0.1 dex today.
Simulation analysis finds ICL mostly from stripped intermediate-mass galaxies and BCGs from massive mergers, with overlapping but non-identical progenitors and distinct mass fractions, colors, and metallicities.
citing papers explorer
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The habitability trade-off: Chemical decoupling and quenching in massive galaxies
Chemically decoupled massive galaxies in IllustrisTNG dominate the high end of a present-day habitability proxy by over an order of magnitude due to a trade-off between suppressed planet formation and reduced sterilizing events.
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Blueberry and Green Pea galaxies live in low density environments
Green Pea and Blueberry galaxies live in isolated low-density environments with the lowest neighbor counts among compared galaxy populations.
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Cluster-green galaxy correlations: where do these galaxies live?
Green valley galaxies live preferentially in the outskirts of galaxy clusters as satellites, consistent with environmental quenching processes.
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Cosmic Environment as the Primary Driver of Dwarf Satellite Statistics
Simulations show dense environments suppress dwarf satellite abundance relative to voids, with environment as the main driver over host stellar mass and morphology.
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Stellar halos of bright central galaxies II: Scaling relations, colors and metallicity evolution with redshift
Stellar halos act as transition regions between bright central galaxies and intracluster light, with strong mass correlations, similar colors that redden over time, and a shrinking metallicity gap from 0.4 dex at z=2 to 0.1 dex today.
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Coevolution of Intracluster Light and Brightest Cluster Galaxies
Simulation analysis finds ICL mostly from stripped intermediate-mass galaxies and BCGs from massive mergers, with overlapping but non-identical progenitors and distinct mass fractions, colors, and metallicities.