Extended [CII] emission reveals a large cold gas halo around the z=7.27 quiescent galaxy RUBIES-UDS-QG-z7, with gas mass estimates indicating f_gas >20% and possible past AGN-driven outflow.
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Detection of [NeV]λ3427 in six recently quenched high-redshift galaxies reveals quasar-like SMBH activity persisting 100-200 Myr after the main quenching epoch.
ArkenstoneBH is a new subgrid model for the hot phase of black hole feedback that, in isolated galaxy tests, suppresses star formation by counteracting gas inflows from the circumgalactic medium.
citing papers explorer
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Extended [CII] gas emission in and around a massive quiescent galaxy at z=7.3
Extended [CII] emission reveals a large cold gas halo around the z=7.27 quiescent galaxy RUBIES-UDS-QG-z7, with gas mass estimates indicating f_gas >20% and possible past AGN-driven outflow.
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High-ionization coronal lines trace quasar-like activity in recently quenched galaxies at high redshift
Detection of [NeV]λ3427 in six recently quenched high-redshift galaxies reveals quasar-like SMBH activity persisting 100-200 Myr after the main quenching epoch.
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ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
ArkenstoneBH is a new subgrid model for the hot phase of black hole feedback that, in isolated galaxy tests, suppresses star formation by counteracting gas inflows from the circumgalactic medium.