Self-gravity in collapsar models produces temporary jet quenching, narrower jets, and modified timescales compared to non-self-gravitating cases, potentially explaining GRB variability and failed bursts.
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Spectral index maps of the limb-brightened jet in 3C 84 show significant evolution across three epochs, indicating dynamic filamentary structures, evolving magnetic fields, and interaction with the ambient medium.
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Three-dimensional GRMHD simulations of jet formation and propagation in self-gravitating collapsing stars
Self-gravity in collapsar models produces temporary jet quenching, narrower jets, and modified timescales compared to non-self-gravitating cases, potentially explaining GRB variability and failed bursts.
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Spectral index evolution of the limb-brightened jet in 3C 84
Spectral index maps of the limb-brightened jet in 3C 84 show significant evolution across three epochs, indicating dynamic filamentary structures, evolving magnetic fields, and interaction with the ambient medium.