Quiescent fractions reach ~50% in hot-accretion high-z groups and ~0% in cold-accretion ones, supporting accretion-mode driven quenching via inside-out starvation.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 2years
2026 2representative citing papers
Simulations demonstrate that mega-parsec giant radio sources form successfully in normal hot baryonic gas environments within 10^13 to 10^15 solar mass dark matter halos, with radio powers matching observations.
citing papers explorer
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Quiescent fractions in high-redshift galaxy groups reflect their hot-or-cold state of gas accretion
Quiescent fractions reach ~50% in hot-accretion high-z groups and ~0% in cold-accretion ones, supporting accretion-mode driven quenching via inside-out starvation.
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Formation of mega-parsec giant radio sources from hosts residing in dark matter halos with normal hot baryonic gas fractions
Simulations demonstrate that mega-parsec giant radio sources form successfully in normal hot baryonic gas environments within 10^13 to 10^15 solar mass dark matter halos, with radio powers matching observations.