Viscous angular-momentum transport and jet feedback can keep intermittent accretion disks around newborn neutron stars alive long enough to launch the energetic jet pairs seen in some supernova remnants.
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Long-lived intermittent accretion disks in the jittering jets explosion mechanism (JJEM) of core-collapse supernovae
Viscous angular-momentum transport and jet feedback can keep intermittent accretion disks around newborn neutron stars alive long enough to launch the energetic jet pairs seen in some supernova remnants.