A z=6.64 LRD host galaxy exhibits a fast AGN-driven outflow with 5500 km/s velocities, dusty gas, and low metallicity, confirming AGN presence in these systems.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Barred galaxies with residual central emission and NUV-r color transition at the bar end represent an intermediate evolutionary phase in bar-driven quenching before full central quenching.
Some LIGO/Virgo BH-BH mergers may arise from black holes in merging ultra-dwarf galaxies at z>1 if merger timescales are 4-7 Gyr, as local rates are too low by an order of magnitude but high-z conditions could match the observed GW rate of 9.7-101 Gpc^-3 yr^-1.
citing papers explorer
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GLIMPSED: Direct evidence for a fast AGN-driven outflow from a z=6.64 Little Red Dot host galaxy
A z=6.64 LRD host galaxy exhibits a fast AGN-driven outflow with 5500 km/s velocities, dusty gas, and low metallicity, confirming AGN presence in these systems.
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Tracing evolutionary pathways of bar-driven quenching in local Universe disc galaxies
Barred galaxies with residual central emission and NUV-r color transition at the bar end represent an intermediate evolutionary phase in bar-driven quenching before full central quenching.
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Gravitational Waves from Black Holes in Merging Ultra-Dwarf Galaxies
Some LIGO/Virgo BH-BH mergers may arise from black holes in merging ultra-dwarf galaxies at z>1 if merger timescales are 4-7 Gyr, as local rates are too low by an order of magnitude but high-z conditions could match the observed GW rate of 9.7-101 Gpc^-3 yr^-1.