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Pulsar Magnetospheres and Pulsar Death [PDF]
Rotating neutron stars, or pulsars, slow down with time. New observations of an unusual intermittent pulsar provide direct evidence that this slowing is partially caused by outflow of plasma.
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2009
Unexpected Encounter What is a Pulsar? Mischievous Ball Misha and Sasha Playing Billiards Stubborn Fountains In the Country of Anisotropic Masses Matter in a Superstrong Magnetic Field Neutron Star Physics of the Pulsar Non-linearity and Self-organization On the Pulsar.
A. Nomerotsky, B. B. Kadomsev
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Unexpected Encounter What is a Pulsar? Mischievous Ball Misha and Sasha Playing Billiards Stubborn Fountains In the Country of Anisotropic Masses Matter in a Superstrong Magnetic Field Neutron Star Physics of the Pulsar Non-linearity and Self-organization On the Pulsar.
A. Nomerotsky, B. B. Kadomsev
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Pulsars and Pulsar Wind Nebulae
2019When heavy stars have burned all their nuclear fuel, neutron degeneracy pressure is the last force able to halt their collapse into a black hole. The sudden stop of the free-fall collapse leads to a rebound of the infalling matter triggering an outward shock that blows up the star envelope and powers a Type II supernova.
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