Journal ArticleDOI
Observation of a Rapidly Pulsating Radio Source
TLDR
In this article, the first report of a curious class of astronomical radio sources, distinguished by their rapid and extremely regular pulsations, was made by Hewish et al. They are now understood to be rapidly rotating, magnetized neutron stars, or pulsars.Abstract:
Unusual signals from pulsating radio sources have been recorded at the Mullard Radio Astronomy Observatory The radiation seems to come from local objects within the galaxy, and may be associated with oscillations of white dwarf or neutron stars 1968 saw the first report of a curious class of astronomical radio sources, distinguished by their rapid and extremely regular pulsations Hewish et al associated them with unusually stable oscillations in compact stars They are now understood to be rapidly rotating, magnetized neutron stars, or pulsarsread more
Citations
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Journal ArticleDOI
Optimal filters for the construction of the ensemble pulsar time
TL;DR: In this article, an algorithm of the ensemble pulsar time based on the optimal Wiener filtration method has been constructed, which allows the separation of the contributions to the post-fit pulsar timing residuals of the atomic clock and the pulsar itself.
Journal ArticleDOI
History of Astroparticle Physics and its Components
TL;DR: An outline of the historical events that led to the formation of contemporary astroparticle physics is given and a brief survey of the most important fields that have played a role in the development of astroparticles physics as the authors know it today is given.
Journal ArticleDOI
Realfast: Real-Time, Commensal Fast Transient Surveys with the Very Large Array.
Casey J. Law,Geoffrey C. Bower,Sarah Burke-Spolaor,Bryan J. Butler,Paul Demorest,A. Halle,Shakeh E. Khudikyan,T. J. W. Lazio,Martin Pokorny,James Robnett,Michael P. Rupen +10 more
TL;DR: Realfast as discussed by the authors is a commensal, fast transient search system at the Jansky Very Large Array (JVL) that uses a novel architecture to distribute fast-sampled interferometric data to a 32-node, 64-GPU cluster.
Journal ArticleDOI
Modelling double neutron stars: radio and gravitational waves
TL;DR: In this paper, a detailed analysis of the double neutron star (DNS) population, accounting for radio survey selection effects, was performed, and a best-fit model that is in broad agreement with the observed Galactic DNS population was proposed.
Gamma-Ray Pulsars
TL;DR: In this paper, a radio telescope at 81.5 MHz was used to study the properties of these cosmic plasma clouds, and a high-speed recorder was fitted with a highspeed recorder to record the intensity of celestial sources passing over the fixed field of radio receivers.
References
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Journal ArticleDOI
Interplanetary Scintillation of Small Diameter Radio Sources
TL;DR: In this article, the authors used the black-body equations to calculate the increased radiation appropriate to the observed brightness increase in the star over a 1,000 A.u. band-width at 5,400 A.U.
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Normal modes of radial pulsation of stars at the end point of thermonuclear evolution
David W. Meltzer,Kip S. Thorne +1 more
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Energetic Particles from the Sun
C. E. Fichtel,F. B. Mcdonald +1 more
TL;DR: In this article, the authors discuss the association of solar cosmic rays with flare association, solar particle acceleration, recurrence and low energy solar particle events, and discuss the effects of solar particle particle acceleration.
Journal ArticleDOI
Possible magnetospheric phenomena associated with neutron stars
TL;DR: In this paper, it was shown that the importance of the early cooling by emission of neutrinos from the Urca process has been underestimated in the foregoing investigations, and the calculations of Miss Tsuruta indicate that a neutron star will rapidly cool to 3 or 4 × 106 °K, but that after 105 years its surface temperature will still be about 2 × 106°K.