Classification of pulsars into bimodal kick modes shows low-B objects overabundant in the low-velocity mode, with no high-velocity examples below 10^11 G.
Core-Collapse Supernovae and Neutron Star Kicks
1 Pith paper cite this work. Polarity classification is still indexing.
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Pith paper citing it
abstract
Recent observations have revealed many new puzzles related to core-collapse supernovae, including the formation of magnetars and black holes and their possible GRB connections. We review our current understanding of the origin of pulsar kicks and supernova asymmetry. It is argued that neutron star kicks are intimately connected to the other fundamental parameters of young neutron stars, such as the initial spin and magnetic field strength.
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astro-ph.HE 1years
2026 1verdicts
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Kick bimodality of neutron stars and mode dependence of their parameters
Classification of pulsars into bimodal kick modes shows low-B objects overabundant in the low-velocity mode, with no high-velocity examples below 10^11 G.