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Induced Rotation in 3D Simulations of Core Collapse Supernovae: Implications for Pulsar Spins
Induced Rotation 3D Simulations Core Collapse Supernovae
2011/1/11
It has been suggested that the observed rotation periods of radio pulsars might be induced by a non-axisymmetric spiral-mode instability in the turbulent region behind the stalled supernova bounce sho...
3D Simulations of the Fragmentation of Photoevaporating Clumps Embedded in a Stellar Wind
3D Simulations Stellar Wind Photoevaporating Clumps Embedded
2009/6/25
3D Simulations of the Fragmentation of Photoevaporating Clumps Embedded in a Stellar Wind。