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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JWST data on SNR 0540-69.3 reveals point-symmetric ejecta morphology consistent with shaping by at least three jet pairs, supporting the jittering-jets explosion mechanism.
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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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JWST observations support the jittering-jets explosion mechanism (JJEM) for the core-collapse supernova remnant SNR 0540-69.3
JWST data on SNR 0540-69.3 reveals point-symmetric ejecta morphology consistent with shaping by at least three jet pairs, supporting the jittering-jets explosion mechanism.
- Reproducing morphological features in the supernova remnant G11.2-0.3 by simulating jittering jets