Results 21 to 30 of about 17,684 (219)
, 2005 We present the results of a large-area survey for millisecond pulsars (MSPs) at moderately high galactic latitudes with the 64 m Parkes radio telescope, along with follow-up timing and optical studies of the newly-discovered pulsars and several others ...
Jacoby, Bryan Anthony
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The Pulsar Wind Nebula of the Geminga Pulsar
The Astrophysical Journal, 2006 Revised version: data analysis described in more detail, Figure 2 replaced; 6 pages, 2 color figures; accepted for publication in ApJ (v.643, 2006 June 1)
Pavlov, G. G., Sanwal, D., Zavlin, V. E.
openaire +2 more sources
Pulsar Polar Cap and Slot Gap Models: Confronting Fermi Data [PDF]
Journal of Astronomy and Space Sciences, 2013 Rotation-powered pulsars are excellent laboratories for studying particle acceleration as well as fundamental physics of strong gravity, strong magnetic fields and relativity.
Alice K. Harding
doaj +1 more source
Classification of unassociated fermi-LAT sources [PDF]
ITM Web of Conferences, 2022 The Large Area Telescope (LAT) on board NASA’s Fermi Gamma-ray Space telescope has detected 5788 sources in the 4FGL catalogue. Among them, 271 have been associated to pulsars, 3436 to blazars, and 1782 remain unassociated sources.
Meng Qiyu
doaj +1 more source
Gravitoastronomy with neutron stars [PDF]
, 2004 Recent advances in gravitational wave detectors mean that we can start to make astrophysically important statements about the physics of neutron stars based on observed upper limits to their gravitational luminosity.
Woan, G., Graham Woan
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Satellite Navigation System with Pulsars. [PDF]
, 2022 The purpose of this thesis is to investigate the feasibility of a navigation system for satellite aided with pulsars. Pulsar navigation system can provide an autonomous method for the determination of position, velocity and attitude of spacecraft for any
Brotto, Francesca
core
The Galactic population of canonical pulsars
, 2022 International audienceCurrent wisdom accounts to the diversity of neutron star observational manifestations to their birth scenarios, influencing their thermal and magnetic field evolution.
Ludmilla Dirson +5 more
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International Journal of Modern Physics D, 2006 Pulsars are wonderful gravitational probes. Their tiny size and stellar mass give their rotation periods a stability comparable to that of atomic frequency standards. This is especially true of the rapidly rotating "millisecond pulsars" (MSPs). Many of these rapidly rotating pulsars are in orbit with another star, allowing pulsar timing to probe ...
openaire +3 more sources
A relativistic navigation system for space [PDF]
, 2011 We present here a method for the relativistic positioning in spacetime based on the reception of pulses from sources of electromagnetic signals whose worldline is known.
Capolongo, Emiliano +6 more
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CIRA-Pulsars-and-Transients-Group/vcstools: Improved Profile Fitting
, 2021 Improvements: Updated how the on-pulse region is determined for profile fitting. This means we can more accurately estimate the S/N. Implemented an exponential-convolved gaussian for fitting so that scattered profiles can be fit more effectively. Added
Sam McSweeney +8 more
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