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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Higher-resolution MUSE data shows the optical torus in SNR E0102 as a multiphase cavity whose line ratios require coexisting shock and ionization conditions rather than any single-component model.
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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A MUSE View of the Optical Torus within the Supernova Remnant 1E 0102.2-7219
Higher-resolution MUSE data shows the optical torus in SNR E0102 as a multiphase cavity whose line ratios require coexisting shock and ionization conditions rather than any single-component model.
- Reproducing morphological features in the supernova remnant G11.2-0.3 by simulating jittering jets