Results 131 to 140 of about 111,592 (291)
Millisecond pulsars are subject to accelerations in globular clusters (GCs) that manifest themselves in both the first and second spin period time derivatives, and can be used to explore the mass distribution of the potentials they inhabit.
A. Corongiu +11 more
doaj +1 more source
In this study, we report on the broadband polarization behavior of the millisecond pulsar B1937+21 (J1939+2134), using high-quality observations made with the ultrawideband low receiver on Murriyang, the Parkes radio telescope.
Z. Wang +7 more
doaj +1 more source
Investigating Unassociated Fermi-LAT sources for the search of Gamma ray pulsars including Millisecond pulsars using semicoherent approch [PDF]
The search for gamma-ray pulsars including millisecond pulsars (MSPs) among unassociated Fermi-Large Area Telescope (LAT) sources offers an opportunity to study these rapidly rotating, highly magnetized neutron stars.
Hrishikesh Chandana A. +5 more
doaj +1 more source
Follow-up Investigation of 11 Pulsars Discovered in the Commensal Radio Astronomy FAST Survey
In this paper, we study 11 pulsars that were discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) in the Commensal Radio Astronomy FAST Survey.
K. Yang +42 more
doaj +1 more source
Follow-up Timing of 12 Pulsars Discovered in Commensal Radio Astronomy FAST Survey
We present phase-connected timing ephemerides, polarization pulse profiles, and Faraday rotation measurements of 12 pulsars discovered by the Five-hundred-meter Aperture Spherical radio Telescope (FAST) in the Commensal Radio Astronomy FAST Survey.
D. Zhao +42 more
doaj +1 more source
Orbital spin dynamics of a millisecond pulsar around a massive BH with a general mass quadrupole [PDF]
Tom Kimpson, Kinwah Wu, Silvia Zane
openalex +1 more source
Are millisecond pulsars different than “Normal” pulsars? [PDF]
AbstractWhile millisecond pulsars have very different period parameters and a different evolutionary history compared to “normal” pulsars, the properties of their pulsed emission are remarkably similar to those of normal pulsars.
openaire +1 more source
The Anomalous Acceleration of PSR J2043+1711: Long-period Orbital Companion or Stellar Flyby?
Based on the rate of change of its orbital period, PSR J2043+1711 has a substantial peculiar acceleration of 3.5 ± 0.8 mm s ^–1 yr ^–1 , which deviates from the acceleration predicted by equilibrium Milky Way (MW) models at a 4 σ level.
Thomas Donlon II +55 more
doaj +1 more source
Full polar cap cascade scenario: $\gamma$-ray and X-ray luminosities from spin-powered pulsars
We modify polar cap cascade picture to include the ICS of the higher generation pairs. In such a ``full-cascade'' scenario, not only the perpendicular portion of the energy of the pairs goes to high energy radiation via SR, but the parallel portion of ...
Alice K. Harding +19 more
core +1 more source
New millisecond pulsars in globular clusters
Paper presented at the 20th Texas Symposium on Relativistic Astrophysics, 10-15 December 2000 - Austin ...
D'AMICO, NICOLO' +5 more
openaire +3 more sources

