A triple-star channel with two common envelope evolution phases produces merging black hole binaries with positive average χ_eff and a tail of negative values.
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6 Pith papers cite this work. Polarity classification is still indexing.
6
Pith papers citing it
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2026 6verdicts
UNVERDICTED 6representative citing papers
Classification of pulsars into bimodal kick modes shows low-B objects overabundant in the low-velocity mode, with no high-velocity examples below 10^11 G.
Depositing stellar luminosity in an inner shell and cooling low-density outer cells produces a stable pulsating 3D red supergiant model for common envelope simulations without relaxation.
Scintillation study of PSR B1257+12 finds distant scattering screens at 166-354 pc and a relatively clean immediate pulsar environment.
Hydrodynamic simulations of three pairs of jittering jets in a CCSN reproduce the ring-and-bar morphology of SNR G11.2-0.3.
FAST observations of three pulsars detect scintillation arcs whose curvatures scale as ν^{-2} with frequency, locating scattering screens at 30-420 pc.
citing papers explorer
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Stellar black hole binaries from two common envelope evolution phases in triple stellar systems
A triple-star channel with two common envelope evolution phases produces merging black hole binaries with positive average χ_eff and a tail of negative values.
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Kick bimodality of neutron stars and mode dependence of their parameters
Classification of pulsars into bimodal kick modes shows low-B objects overabundant in the low-velocity mode, with no high-velocity examples below 10^11 G.
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Scintillation of the first-known pulsar planetary system
Scintillation study of PSR B1257+12 finds distant scattering screens at 166-354 pc and a relatively clean immediate pulsar environment.
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Reproducing morphological features in the supernova remnant G11.2-0.3 by simulating jittering jets
Hydrodynamic simulations of three pairs of jittering jets in a CCSN reproduce the ring-and-bar morphology of SNR G11.2-0.3.
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Interstellar Scintillation of Three Nearby Pulsars with FAST
FAST observations of three pulsars detect scintillation arcs whose curvatures scale as ν^{-2} with frequency, locating scattering screens at 30-420 pc.