Results 111 to 120 of about 5,319 (222)

Radio polarimetry of Galactic Centre pulsars

open access: yes, 2016
To study the strength and structure of the magnetic field in the Galactic Centre (GC), we measured Faraday rotation of the radio emission of pulsars which are seen towards the GC.
Eatough, R. P.   +18 more
core   +1 more source

The radio luminosity distribution of pulsars in 47 Tucanae

open access: yes, 2004
Restricted Access. An open access version is available at arXiv.org.We have used the Australia Telescope Compact Array to seek the integrated radio flux from all the pulsars in the core of the globular cluster 47 Tucanae.
Connors, T.   +3 more
core   +1 more source

The radio lighthouse from afar: In search of distant pulsars [PDF]

open access: yes, 2018
Modern radio-pulsar catalogues contain a large diversity of objects: young solitary pulsars and old ones in binary systems, periodic or sporadic emitters; bright and magnetized, or faint and even eclipsing.
Mikhailov, K.V.
core   +1 more source

On the Difference between Pulsar Radio Emission Beams from the Two Poles

open access: yesThe Astrophysical Journal
The long-standing assumption of symmetric radio emission beams from the two magnetic poles of pulsars is challenged by observational evidence of asymmetry and underfill. Direct testing of this symmetry remains difficult for most pulsars.
Xiancong Wu   +6 more
doaj   +1 more source

Radio pulsars with expected gamma radiation and gamma pulsars as pulsating radio emitters [PDF]

open access: yes, 2018
Мы показали, что радиопульсары, обнаруженные в виде источников импульсного гамма-излучения на Ферми/ЛАТ, имеют очень высокие значения магнитного поля вблизи светового цилиндра и скорости потери энергии вращения.
Тимиркеева, М. А.   +1 more
core  

Timing of Millisecond Pulsars in NGC 6752. III. On the Presence of Nonluminous Matter in the Cluster’s Core

open access: yesThe Astrophysical Journal
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

A binary pulsar in a 53-minute orbit. [PDF]

open access: yesNature, 2023
Pan Z   +17 more
europepmc   +1 more source

Radio Pulsar Populations

open access: yes, 2019
Astro2020 white paper (submitted to the NASA 2020 astronomy and astrophysics decadal survey)
Lorimer, D. R.   +11 more
openaire   +2 more sources

A Search for Radio-Quiet Gamma-Ray Pulsars [PDF]

open access: yes, 2000
Most Galactic point sources of gamma rays remain unidentified. The few (extrasolar) sources that have been identified are all young, rotation-powered pulsars, all but one of which were identified using radio ephemerides.
Koh, D. T.   +6 more
core  

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