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The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars
We present 294 pulsars found in GeV data from the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope. Another 33 millisecond pulsars (MSPs) discovered in deep radio searches of LAT sources will likely reveal pulsations once phase-connected
D. A. Smith+170 more
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Gravity Tests with Radio Pulsars
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
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Magnetic fields of radio pulsars [PDF]
The mechanism of magnetodipole braking of radio pulsars is used to calculate new values of the surface magnetic fields of neutron stars. The angles β between the spin axes and magnetic moments of the neutron stars were estimated for 376 radio pulsars ...
E. B. Nikitina, I. Malov
semanticscholar +5 more sources
Almost 50 years after radio pulsars were discovered in 1967, our understanding of these objects remains incomplete. On the one hand, within a few years it became clear that neutron star rotation gives rise to the extremely stable sequence of radio pulses,
V. S. Beskin+3 more
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Timing of young radio pulsars – I. Timing noise, periodic modulation, and proper motion [PDF]
The smooth spin-down of young pulsars is perturbed by two non-deterministic phenomenon, glitches, and timing noise. Although the timing noise provides insights into nuclear and plasma physics at extreme densities, it acts as a barrier to high-precision
S Johnston, P Weltevrede, W Van Straten
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14 pages, Latex, aas2pp4.sty, To appear in Satellite and Ground Based Studies of Radio Pulsars, proceedings of the 31st Scientific Assembly of ...
J. F. Bell
openalex +5 more sources
Gravity experiments with radio pulsars [PDF]
The discovery of the first pulsar in a binary star system, the Hulse–Taylor pulsar, 50 years ago opened up an entirely new field of experimental gravity.
Paulo C. C. Freire, N. Wex
semanticscholar +4 more sources
RADIO EFFICIENCY OF PULSARS [PDF]
We investigate radio emission efficiency, ξ, of pulsars and report a near-linear inverse correlation between ξ and the spin-down power, , as well as a near-linear correlation between ξ and pulsar age, τ.
A. Szary+4 more
semanticscholar +5 more sources
Constraining the dense matter equation-of-state with radio pulsars [PDF]
Radio pulsars provide some of the most important constraints for our understanding of matter at supranuclear densities. So far, these constraints are mostly given by precision mass measurements of neutron stars (NS). By combining single measurements of
Huanchen Hu+4 more
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