Results 121 to 130 of about 76,238 (239)

Neutron star mass estimates from gamma-ray eclipses in spider millisecond pulsar binaries. [PDF]

open access: yesNat Astron, 2023
Clark CJ   +28 more
europepmc   +1 more source

The Origin of the Binary Pulsar J0737-3039 [PDF]

open access: green, 2005
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]

open access: green, 2023
P. P. Li   +22 more
openalex   +1 more source

Prediction of Radio-quiet Gamma-Ray Pulsar Distances Using the Fundamental Plane Relation

open access: yesThe Astrophysical Journal
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

The optical counterparts of accreting millisecond X-ray pulsars during quiescence [PDF]

open access: bronze, 2009
P. D'Avanzo   +5 more
openalex   +1 more source

Arecibo HiAbsorption Measurements of Pulsars and the Electron Density at Intermediate Longitudes in the First Galactic Quadrant [PDF]

open access: bronze, 2008
J. M. Weisberg   +6 more
openalex   +1 more source

Pulsar magnetic alignment: a classification of pulsars [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1977
openaire   +2 more sources

Pulsar Gleaners: Discovery of 19 Pulsars in FAST Archival Data at ∣b∣ < 5° and Decl. < −5°

open access: yesThe Astrophysical Journal
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

open access: yesThe Astrophysical Journal
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

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