Results 61 to 70 of about 16,242 (188)
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
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
Reassessing The Fundamentals: New Constraints on the Evolution, Ages and Masses of Neutron Stars
The ages and masses of neutron stars (NSs) are two fundamental threads that make pulsars accessible to other sub-disciplines of astronomy and physics.
Kiziltan, Bulent
core +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
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
Outer gap accelerator closed by magnetic pair-creation process
We discuss outer gap closure mechanism in the trans-field direction with the magnetic pair-creation process near the stellar surface. The gap closure by the magnetic pair-creation is possible if some fraction of the pairs are produced with an outgoing ...
Abdo +21 more
core +1 more source
Can eccentric binary millisecond pulsars form by accretion induced collapse of white dwarfs?
Binary radio pulsars are generally believed to have been spun up to millisecond periods (i.e. recycling) via mass accretion from their donor stars, and they are the descendants of neutron star low-mass X-ray binaries.
Alpar +55 more
core +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
Machine learning, algorithms to extract empirical knowledge from data, can be used to classify data, which is one of the most common tasks in observational astronomy.
Abdo +22 more
core +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

