Cold CGM clouds under quasar radiation follow optically thin ionization, radiation-shielded, or rocket-effect paths, with the latter increasing Lyα luminosity up to 10x and bright quasars fully ionizing the cold gas while faint ones drive rocket effects.
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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 find that tidal dwarf galaxies form and persist in galaxy clusters under moderate stellar feedback across all relevant viscosities, supporting their identification as stripped remnants matching multiple observed dwarf galaxy classes.
citing papers explorer
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The hydrodynamical response of cold circumgalactic clouds to quasar radiation
Cold CGM clouds under quasar radiation follow optically thin ionization, radiation-shielded, or rocket-effect paths, with the latter increasing Lyα luminosity up to 10x and bright quasars fully ionizing the cold gas while faint ones drive rocket effects.
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Merge and Strip II: Imprint of galaxy formation physics and viscosity on baryon-dominated dwarf galaxies
Simulations find that tidal dwarf galaxies form and persist in galaxy clusters under moderate stellar feedback across all relevant viscosities, supporting their identification as stripped remnants matching multiple observed dwarf galaxy classes.