Observational discovery of an overmassive, highly accreting black hole in the secondary galaxy of a high-redshift minor merger, providing evidence that such mergers can drive rapid BH growth.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Seyfert galaxy slab coronae show a nearly constant Compton y-parameter of 0.414, implying regulation by slab radiative equilibrium.
citing papers explorer
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Minor Merger, Major Growth: An Overmassive, Highly Accreting Black Hole Powering a Secondary AGN In a Cosmic Noon Minor Merger
Observational discovery of an overmassive, highly accreting black hole in the secondary galaxy of a high-redshift minor merger, providing evidence that such mergers can drive rapid BH growth.
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A Nearly Constant Compton y-parameter for Mildly Relativistic Slab Coronae in AGN
Seyfert galaxy slab coronae show a nearly constant Compton y-parameter of 0.414, implying regulation by slab radiative equilibrium.