Sweeping secular resonance from an intermediate-mass companion and depleting disk enhances AGN TDE rates to 10^{-3}-10^{-2} per galaxy per year on Myr timescales.
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6 Pith papers cite this work. Polarity classification is still indexing.
6
Pith papers citing it
representative citing papers
Swift J1727.8-1613 shows a positive correlation between energy-dependent time lag and X-ray polarization degree in a type-C QPO, which may require additional emission processes.
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.
Accretion increases observable water mass in disks by expanding the emitting area via higher central luminosity, while viscous heating has no effect.
Accretion feedback caps stellar growth rates below 0.1 solar masses per year in AGN disks, eliminates runaway accretion, and produces higher equilibrium masses and luminosities when gap opening is included.
Chandra HETG spectroscopy of BZ Cam diagnoses an ADAF-like advective hot flow with plasma densities of a few times 10^12-14 cm^-3, temperatures of 3-30 million K, and nonequilibrium ionization conditions.
citing papers explorer
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Enhancement of the Rate of Tidal Disruption Events in Active Galactic Nuclei due to the Sweeping Secular Resonance Mechanism
Sweeping secular resonance from an intermediate-mass companion and depleting disk enhances AGN TDE rates to 10^{-3}-10^{-2} per galaxy per year on Myr timescales.
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Bridging X-ray Polarization with Timing & Spectroscopic Parameters of a galactic black hole: Swift J1727.8-1613
Swift J1727.8-1613 shows a positive correlation between energy-dependent time lag and X-ray polarization degree in a type-C QPO, which may require additional emission processes.
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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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JWST-DECO: The Impact of Accretion on Mid-Infrared Observable Water in Planet-forming Disks
Accretion increases observable water mass in disks by expanding the emitting area via higher central luminosity, while viscous heating has no effect.
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The Effects of Accretion Feedback on Stellar Evolution in AGN Disks
Accretion feedback caps stellar growth rates below 0.1 solar masses per year in AGN disks, eliminates runaway accretion, and produces higher equilibrium masses and luminosities when gap opening is included.
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High Resolution X-ray Spectroscopy of the Nova-Like Cataclysmic Variable BZ Cam using Chandra HETG: Diagnosis of the ADAF-like (Advective) Hot Flow
Chandra HETG spectroscopy of BZ Cam diagnoses an ADAF-like advective hot flow with plasma densities of a few times 10^12-14 cm^-3, temperatures of 3-30 million K, and nonequilibrium ionization conditions.