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Pulsars [PDF]

open access: yesPhysics Today, 1968
THE DISCOVERY OF PULSARS, or rapidly pulsating radio sources, was, like certain other historic events in astronomy, an accident. It is reminiscent of the unexpected detection of radio bursts from Jupiter by Bernard F. Burke and Kenneth L. Franklin, who were studying the Crab Nebula, and of the discovery of the cosmic fireball radiation by Arno A ...
Stephen P. Maran, A. G. W. Cameron
  +4 more sources

The Galactic Millisecond Pulsar Population [PDF]

open access: yes, 2012
Among the current sample of over 2000 radio pulsars known primarily in the disk of our Galaxy, millisecond pulsars now number almost 200. Due to the phenomenal success of blind surveys of the Galactic field, and targeted searches of Fermi gamma-ray ...
Lorimer, Duncan R.
core   +1 more source

Gravity Tests with Radio Pulsars

open access: yesUniverse, 2020
The discovery of the first binary pulsar in 1974 has opened up a completely new field of experimental gravity. In numerous important ways, pulsars have taken precision gravity tests quantitatively and qualitatively beyond the weak-field slow-motion ...
Norbert Wex, Michael Kramer
doaj   +1 more source

Post-main-sequence planetary system evolution [PDF]

open access: yesRoyal Society Open Science, 2016
The fates of planetary systems provide unassailable insights into their formation and represent rich cross-disciplinary dynamical laboratories. Mounting observations of post-main-sequence planetary systems necessitate a complementary level of theoretical
Dimitri Veras
doaj   +1 more source

The observed velocity distribution of young pulsars [PDF]

open access: yes, 2017
We argue that comparison with observations of theoretical models for the velocity distribution of pulsars must be done directly with the observed quantities, i.e. parallax and the two components of proper motion.
Cator, Eric   +2 more
core   +2 more sources

The effect of small inter-pulsar distance variations in stochastic gravitational wave background searches with Pulsar Timing Arrays [PDF]

open access: yes, 2014
One of the primary objectives for Pulsar Timing Arrays (PTAs) is to detect a stochastic background generated by the incoherent superposition of gravitational waves (GWs), in particular from the cosmic population of supermassive black hole binaries ...
Mingarelli, Chiara M. F., Sidery, Trevor
core   +3 more sources

Gravitational waves from pulsars in the context of magnetic ellipticity

open access: yesEuropean Physical Journal C: Particles and Fields, 2017
In one of our previous articles we have considered the role of a time dependent magnetic ellipticity on the pulsars’ braking indices and on the putative gravitational waves these objects can emit.
José C. N. de Araujo   +2 more
doaj   +1 more source

Pulsar Physics and GLAST [PDF]

open access: yes, 2007
Rotation-powered pulsars are excellent laboratories for study of particle acceleration as well as fundamental physics of strong gravity, strong magnetic fields, high densities and relativity.
Harding, Alice K.
core   +2 more sources

Pulsar Polar Cap and Slot Gap Models: Confronting Fermi Data [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2013
Rotation-powered pulsars are excellent laboratories for studying particle acceleration as well as fundamental physics of strong gravity, strong magnetic fields and relativity.
Alice K. Harding
doaj   +1 more source

Finding pulsars with LOFAR [PDF]

open access: yes, 2007
We investigate the number and type of pulsars that will be discovered with the low-frequency radio telescope LOFAR. We consider different search strategies for the Galaxy, for globular clusters and for galaxies other than our own.
Stappers, Ben, van Leeuwen, Joeri
core   +2 more sources

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