Results 141 to 150 of about 1,603 (188)
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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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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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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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