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Space Science Reviews, 1994
25 years after their discovery, pulsars still pose fundamental problems, in particular when the whole range of their periodsP is considered: 1.56 ms ≤P≤0.09 s. This communication reviews my understanding of the pulsar magnetosphere, windzone, and (coherent) radio emission.
Hsiang-Kuang Chang, Wolfgang Kundt
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25 years after their discovery, pulsars still pose fundamental problems, in particular when the whole range of their periodsP is considered: 1.56 ms ≤P≤0.09 s. This communication reviews my understanding of the pulsar magnetosphere, windzone, and (coherent) radio emission.
Hsiang-Kuang Chang, Wolfgang Kundt
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A new version of the theory of pulsar radio emission is developed for the case of a coaxial rotator. It is based on the electric field that we established [G. S. Sahakian, Astrofizika, 37, 97 (1994)] for the radiation channel (the channel of open magnetic field lines) and on convenient approximations for the electron energy obtained in [G. S.
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Magneto–Thermal Evolution of Neutron Stars with Emphasis to Radio Pulsars
Journal of astrophysics and astronomy, 2017The magnetic and thermal evolution of neutron stars is a very complex process with many non-linear interactions. For a decent understanding of neutron star physics, these evolutions cannot be considered isolated.
U. Geppert
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AbstractA review of simultaneous and compiled spectra is presented, and a catalog of radio spectra for 340 pulsars reported. Pulsars with flux density measurements at three and more frequencies are included. Statistics of spectral indices and frequencies of the energy maximum and the break are presented, as well as the correlations with other pulsar ...
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2006
Radio pulsars are a major probe of the Galactic neutron star population and its evolution. Our attempts to derive the properties of the underlying, as opposed to the observed, population of radio pulsars in our Galaxy have gradually improved over the years thanks to large-scale surveys and more detailed simulations of the population.
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Radio pulsars are a major probe of the Galactic neutron star population and its evolution. Our attempts to derive the properties of the underlying, as opposed to the observed, population of radio pulsars in our Galaxy have gradually improved over the years thanks to large-scale surveys and more detailed simulations of the population.
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New Astronomy, 1998
Abstract We report the results of our search for pulsed radio emission from Geminga carried out in 1992, 1993 and 1996–1997 at 102.5 MHz using the BSA radiotelescope of the Pushchino Radioastronomy Observatory. The Geminga radio pulsar (PSR J0633+1746) was detected in all three observation periods.
V. D. Pugachev, Yu. P. Shitov
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Abstract We report the results of our search for pulsed radio emission from Geminga carried out in 1992, 1993 and 1996–1997 at 102.5 MHz using the BSA radiotelescope of the Pushchino Radioastronomy Observatory. The Geminga radio pulsar (PSR J0633+1746) was detected in all three observation periods.
V. D. Pugachev, Yu. P. Shitov
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Generation of Radio Waves in Pulsars [PDF]
Pulsars generate radio waves by an unknown process which gives the highest volume emissivity known in astrophysics. The radiation forms a beam the width and polarization of which are independent of frequency. This article assembles the observational facts which any theory of emission must explain.
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