A relativistic funnel scattering model with variable bulk velocity reproduces the ~23% hard-state and ~12% soft-state polarization in Cygnus X-3 at low inclination using half-opening angles of 13-16 degrees.
10.1051/0004-6361/202451356
6 Pith papers cite this work, alongside 23 external citations. Polarity classification is still indexing.
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representative citing papers
Full-transport radiation GRMHD simulations show super-Eddington black hole accretion is geometrically thick, drives strong outflows, and radiates with very low efficiency (below about 0.5% at 150 times Eddington).
A semi-analytic model shows dense early star clusters can grow 1000-solar-mass black hole seeds to ~10^7 solar masses within ~100 million years, predicting tens of tidal disruptions per year from Little Red Dots at z=4-6.
The counterjet dominates PeV photon production in Cyg X-3 due to longer interaction paths through the donor star's wind at low inclination.
A new IXPE observation finds no X-ray polarization from MAXI J1744-294 and uses the 1.3% upper limit to constrain the accretion disk inclination to roughly 38-71 degrees, depending on spin and atmosphere albedo.
IXPE, launched in December 2021, is the first dedicated imaging X-ray polarimetry observatory and has measured X-ray polarization for about 110 cosmic sources.
citing papers explorer
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Relativistic Scattering in the Funnel of Cygnus X-3
A relativistic funnel scattering model with variable bulk velocity reproduces the ~23% hard-state and ~12% soft-state polarization in Cygnus X-3 at low inclination using half-opening angles of 13-16 degrees.
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Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: I. Survey of Eddington Ratios
Full-transport radiation GRMHD simulations show super-Eddington black hole accretion is geometrically thick, drives strong outflows, and radiates with very low efficiency (below about 0.5% at 150 times Eddington).
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From nuclear star clusters to Little Red Dots: black hole growth, mergers, and tidal disruptions
A semi-analytic model shows dense early star clusters can grow 1000-solar-mass black hole seeds to ~10^7 solar masses within ~100 million years, predicting tens of tidal disruptions per year from Little Red Dots at z=4-6.
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The counterjet dominates the production of PeV photons from Cyg X-3
The counterjet dominates PeV photon production in Cyg X-3 due to longer interaction paths through the donor star's wind at low inclination.
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Exploring MAXI J1744-294: IXPE insights into a Newly Discovered X-ray Transient
A new IXPE observation finds no X-ray polarization from MAXI J1744-294 and uses the 1.3% upper limit to constrain the accretion disk inclination to roughly 38-71 degrees, depending on spin and atmosphere albedo.