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Observations of the gamma-ray pulsar J1836+5925 at 111 MHz
We describe the 10-day radio observations of the gamma-ray pulsar J1836+5925. Observations were carried out in the Pushchino Radio Astronomical Observatory at the frequency of 111 MHz using the Large Phased Array of the Lebedev Physical Institute.
Timirkeeva Maria+3 more
doaj +1 more source
Pulsar magnetospheres and pulsar winds [PDF]
10 pages, 6 (black and white) figures, in Proceedings of the 2016 Heidelberg Symposium on High Energy Gamma-Ray ...
openaire +3 more sources
The Galactic Millisecond Pulsar Population [PDF]
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
REPEATING FAST RADIO BURSTS FROM HIGHLY MAGNETIZED PULSARS TRAVELING THROUGH ASTEROID BELTS [PDF]
Very recently, Spitler et al. and Scholz et al. reported their detections of 16 additional bright bursts in the direction of the fast radio burst (FRB) 121102.
Z. Dai+3 more
semanticscholar +1 more source
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
doaj +1 more source
Post-main-sequence planetary system evolution [PDF]
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
Fast radio bursts as giant pulses from young rapidly rotating pulsars [PDF]
We discuss possible association of fast radio bursts (FRBs) with supergiant pulses emitted by young pulsars (ages $\sim$ tens to hundreds of years) born with regular magnetic field but very short -- few milliseconds -- spin periods.
M. Lyutikov, L. Burzawa, S. Popov
semanticscholar +1 more source
Polarimetry of 600 pulsars from observations at 1.4 GHz with the Parkes radio telescope [PDF]
Over the past 13 years, the Parkes radio telescope has observed a large number of pulsars using digital filterbank backends with high time and frequency resolution and the capability for Stokes recording.
S. Johnston, M. Kerr
semanticscholar +1 more source
Gravitational waves from pulsars in the context of magnetic ellipticity
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 Polar Cap and Slot Gap Models: Confronting Fermi Data [PDF]
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