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Pulsar Magnetospheres and Pulsar Death
Science, 2006Rotating 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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International Journal of Modern Physics A, 1990
v1.6 We review the theory and observational status of strange-pulsar models. After introduction of the subject, a summary of observational facts about pulsars is presented. The theory of quark matter and strange matter relevant to astrophysical applications is briefly discussed, and applied afterwards to type-II supernova theory and to pulsar models ...
, Benvenuto, , Horvath, , Vucetich
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v1.6 We review the theory and observational status of strange-pulsar models. After introduction of the subject, a summary of observational facts about pulsars is presented. The theory of quark matter and strange matter relevant to astrophysical applications is briefly discussed, and applied afterwards to type-II supernova theory and to pulsar models ...
, Benvenuto, , Horvath, , Vucetich
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Nature Physical Science, 1971
Abstract The energy loss from the neutron star - as inferred from the secular increase in rotation period - is much greater than that emitted in either the radio or the other observed wavelengths. A primary motivation of magnetospheric theory is to trace the mode in which this energy and the associated angular momentum are in fact ...
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Abstract The energy loss from the neutron star - as inferred from the secular increase in rotation period - is much greater than that emitted in either the radio or the other observed wavelengths. A primary motivation of magnetospheric theory is to trace the mode in which this energy and the associated angular momentum are in fact ...
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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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Astrophysics and Space Science, 2000
Domains of the pulsar magnetosphere, both within and without the light-cylinder, are studied under varying provisional assumptions. Some of the qualitative features emerging should persist in the ultimate synthesis of a completely self-consistent model.
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Domains of the pulsar magnetosphere, both within and without the light-cylinder, are studied under varying provisional assumptions. Some of the qualitative features emerging should persist in the ultimate synthesis of a completely self-consistent model.
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1999
Observations of proper motions of single radio pulsars enable the determination of transverse velocities and hence provide a tool for measuring the amount of asymmetry (i. e., the magnitude of the kick velocity vec{w}) in supernovae (SNe). However, single pulsars are thought to originate from both isolated early type stars which explode in a type II SN
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Observations of proper motions of single radio pulsars enable the determination of transverse velocities and hence provide a tool for measuring the amount of asymmetry (i. e., the magnitude of the kick velocity vec{w}) in supernovae (SNe). However, single pulsars are thought to originate from both isolated early type stars which explode in a type II SN
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