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The origin of single radio pulsars [PDF]
New Astron. 4 (1999) 355-363, 1999 By comparing relative rates of supernovae versus formation rates of single radio pulsars, recycled pulsars, binary pulsars and X-ray binaries we put strong limits on the progenitors of radio pulsars and on the requirement of an asymmetry in the supernova.
Edward P. J. van den Heuvel +2 more
arxiv +9 more sources
Radio efficiency of pulsars [PDF]
The Astrophysical Journal, 2014 We investigate radio emission efficiency $\xi$ of pulsars and report a near linear inverse correlation between $\xi$ and the spindown power $\dot E$, as well as a near linear correlation between $\xi$ and pulsar age $\tau$. This is a consequence of very weak, if any, dependences of radio luminosity $L$ on pulsar period $P$ and period derivative $\dot{P}
George I. Melikidze +7 more
arxiv +7 more sources
The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars
The Astrophysical Journal, 2023 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
doaj +2 more sources
Gravity Tests with Radio Pulsars
Universe, 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 +2 more sources
Magnetic fields of radio pulsars [PDF]
Astronomy Reports, 2017 We used the magneto-dipole radiation mechanism for the braking of radio pulsars to calculate the new values of magnetic inductions at the surfaces of neutron stars. For this aim we estimated the angles ? between the rotation axis and the magnetic moment of the neutron star for 376 radio pulsars using three different methods. It was shown that there was
E. B. Nikitina, I. F. Malov
openaire +5 more sources
Space Science Reviews, 2015 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, that the kinetic energy of rotation provides the reservoir of energy, and that electromagnetic ...
Beskin, VS +3 more
openaire +4 more sources
Timing of young radio pulsars – I. Timing noise, periodic modulation, and proper motion [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 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
exaly +2 more sources
Advances in Space Research, 1996 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
Radio pulsars with expected gamma radiation and gamma pulsars as pulsating radio emitters [PDF]
Research in Astronomy and Astrophysics, 2017 Pulsars play a crucial astrophysical role as the highly energetic compact radio, X-ray, and gamma-ray sources. Our previous works show that the radio pulsars found as the pulsing gamma sources by the Large Area Telescope (LAT) on the board of the Fermi Gamma-Ray Space Telescope have high values of magnetic field near the light cylinder, two-three ...
Maria Andreevna Timirkeeva +1 more
arxiv +6 more sources
The shape of pulsar radio beams [PDF]
Monthly Notices of the Royal Astronomical Society, 2001 5 pages, 4 figures.
J. L. Han, R. N. Manchester
openalex +4 more sources