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.
A polarized view of the young pulsar wind nebula 3C 58 with IXPE
4 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
citation-role summary
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citation-polarity summary
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astro-ph.HE 4years
2026 4roles
background 1polarities
background 1representative citing papers
Hydrodynamic simulations of three pairs of jittering jets in a CCSN reproduce the ring-and-bar morphology of SNR G11.2-0.3.
A consolidated IXPE data-analysis recipe, with new post-DU2-anomaly background-rejection thresholds fitted to one observation.
SKA will enable spatially resolved radio studies of pulsar wind nebulae to probe particle acceleration and propagation in ultra-relativistic outflows.
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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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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The hitchhiker's guide to the IXPE data analysis
A consolidated IXPE data-analysis recipe, with new post-DU2-anomaly background-rejection thresholds fitted to one observation.
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Understanding Pulsar Wind Nebulae with the SKA
SKA will enable spatially resolved radio studies of pulsar wind nebulae to probe particle acceleration and propagation in ultra-relativistic outflows.