Spectroscopic and imaging confirmation of the brightest known quadruply-lensed quasar J1330-0905 at z=2.22 with Einstein radius ~0.45 arcsec and predicted magnification ~56.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
representative citing papers
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 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.
citing papers explorer
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Persephone's Torch: A 15th Magnitude Quadruply-Lensed Quasar From the Couch Discovered with SPHEREx and the LBT
Spectroscopic and imaging confirmation of the brightest known quadruply-lensed quasar J1330-0905 at z=2.22 with Einstein radius ~0.45 arcsec and predicted magnification ~56.
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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 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.