Simulations demonstrate that timescale-based decoupling predictions overestimate separations by a factor of ~3, velocity-based criteria are more accurate, and low-viscosity disks produce decreasing accretion that may identify LISA hosts.
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3 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 3representative citing papers
Spectral monitoring indicates NGC 3786's changing-look AGN transition results from torus covering factor variations driven by Eddington ratio and accretion mode changes.
Recovers individual f virial factors from dynamical modeling plus RM data and reports evidence for correlation of log f with black hole mass plus marginal links to BLR thickness, inclination, and line shape.
citing papers explorer
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The Decoupling of Binaries from Their Circumbinary Disks
Simulations demonstrate that timescale-based decoupling predictions overestimate separations by a factor of ~3, velocity-based criteria are more accurate, and low-viscosity disks produce decreasing accretion that may identify LISA hosts.
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The Changing-look Phenomenon Accompanied by an Accretion Mode Transition in NGC 3786
Spectral monitoring indicates NGC 3786's changing-look AGN transition results from torus covering factor variations driven by Eddington ratio and accretion mode changes.
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What Does the Virial Coefficient of the \Hb Broad-Line Region Depend On?
Recovers individual f virial factors from dynamical modeling plus RM data and reports evidence for correlation of log f with black hole mass plus marginal links to BLR thickness, inclination, and line shape.