New 3D simulations show Rayleigh-Taylor instabilities turn jet-driven common-envelope ejecta into filaments, with faster envelope rotation making spiral arms more prominent.
2017b, MNRAS
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Jet-shaped filamentary ejecta in common envelope evolution
New 3D simulations show Rayleigh-Taylor instabilities turn jet-driven common-envelope ejecta into filaments, with faster envelope rotation making spiral arms more prominent.