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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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.