Neutron star mass estimates from gamma-ray eclipses in spider millisecond pulsar binaries. [PDF]
Clark CJ +28 more
europepmc +1 more source
The Origin of the Binary Pulsar J0737-3039 [PDF]
Tsvi Piran, Nir J. Shaviv
openalex +1 more source
Timing properties of the X-ray accreting pulsar RX J0440.9+4431 studied with Insight-HXMT and NICER [PDF]
P. P. Li +22 more
openalex +1 more source
Prediction of Radio-quiet Gamma-Ray Pulsar Distances Using the Fundamental Plane Relation
The fundamental plane (FP) relation connects gamma-ray luminosity to intrinsic pulsar properties, offering the potential to estimate distances for radio-quiet (RQ) gamma-ray pulsars, where direct measurements are often unavailable. The Fermi Third Pulsar
Ekrem Oğuzhan Angüner
doaj +1 more source
AI-powered drone-based automated inspection of FAST. [PDF]
Wang L.
europepmc +1 more source
The optical counterparts of accreting millisecond X-ray pulsars during quiescence [PDF]
P. D'Avanzo +5 more
openalex +1 more source
Arecibo H
J. M. Weisberg +6 more
openalex +1 more source
Pulsar magnetic alignment: a classification of pulsars [PDF]
openaire +2 more sources
Pulsar Gleaners: Discovery of 19 Pulsars in FAST Archival Data at ∣b∣ < 5° and Decl. < −5°
We report the discovery of 19 new pulsars identified from archival observations of the Five-hundred-meter Aperture Spherical radio Telescope (FAST) within Galactic latitudes ∣ b ∣ < 5° and declinations decl. < −5°. The dataset was recorded using FAST’s L
Shi-Jie Gao, Yi-Xuan Shao, Xiang-Dong Li
doaj +1 more source
Single Millisecond Pulsars from Dynamical Interaction Processes in Dense Star Clusters
Globular clusters (GCs) are particularly efficient at forming millisecond pulsars. Among these pulsars, about half lack a companion star, a significantly higher fraction than in the Galactic field.
Claire S. Ye +3 more
doaj +1 more source

