Results 91 to 100 of about 3,272 (170)
Radio Pulse Search from Aql X-1
We present 12 observations of the accreting millisecond X-ray pulsar Aql X-1, taken from 2022 August to 2023 October using the Five-hundred-meter Aperture Spherical Radio Telescope at 1250 MHz.
Long Peng +7 more
doaj +1 more source
One blind and three targeted searches for (sub)millisecond pulsars [PDF]
Context. Millisecond pulsars are very useful for determining the properties of neutron stars, for testing General Relativity and for detecting gravitational waves.
E. Davoust, G. Petit, T. Fayard
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
Spin-Down of Radio Millisecond Pulsars at Genesis [PDF]
Millisecond pulsars are old neutron stars that have been spun up to high rotational frequencies via accretion of mass from a binary companion star. An important issue for understanding the physics of the early spin evolution of millisecond pulsars is the
Tauris, Thomas M.; id_orcid
core +1 more source
On the Number of Confirmed Pulsar Planets: The Rule of Six
Since the first definitive exoplanet detection, the three planets around millisecond radio pulsar PSR B1257+12, few more pulsar planets (PPs) have been reported.
Silas G. T. Laycock +1 more
doaj +1 more source
Spider pulsars represent a unique subclass of radio millisecond pulsars in binaries, and are further categorized into black widows and redbacks according to the mass of the low-mass companion.
Chunyan Lu +5 more
doaj +1 more source
Pulse profile stability in millisecond pulsars (MSPs) is a key factor in achieving high-precision timing essential for detecting nanohertz gravitational waves with pulsar timing arrays (PTAs).
Ankita Ghosh +5 more
doaj +1 more source
Pulse Profile Variability of PSR J1022+1001 in NANOGrav Data
Pulse profile stability is a central assumption of standard pulsar timing methods. Thus, it is important for pulsar timing array experiments such as the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) to account for any pulse ...
William Fiore +48 more
doaj +1 more source

