Results 111 to 120 of about 72,188 (265)

A multiwavelength study on the high-energy behaviour of Fermi/LAT pulsars

, 2011
Using archival as well as freshly acquired data, we assess the X-ray behaviour of the Fermi/LAT gamma-ray pulsars listed in the First Fermi source catalog.
Abdo, Abdo, Abdo, Abdo, Andrea De Luca, Arnaud, Becker, Becker, Bird, Brogan, Camilo, De Luca, Giommi, Gotthelf, Gotthelf, Hales, Halpern, Hwang, Kargaltsev, Kargaltsev, Kaspi, Kaspi, Kaspi, Kothes, Li, Manchester, Martino Marelli, Migliazzo, Mignani, Muslimov, Patrizia A. Caraveo, Ray, Roberts, Saz Parkinson, Slane, Steiner, Stuhlinger, Tam, Thompson, Thorsett, Watters, Winkler, Zhang, Zhang   +43 more
core   +1 more source

Pulsar Electrodynamics

Symposium - International Astronomical Union, 1981
This paper briefly discusses the salient features of quasi-steady electrodynamics; that is to say it considers certain general properties of Maxwell's equations and their solutions when these equations are subjected to the constraint where ω is a constant angular frequency, ⊘ and t are the azimuthal angle and time, and the operators are applied only ...
openaire   +1 more source

Pulsar glitch substructure and pulsar interiors

, 2009
Bursts, Pulses and Flickering: Wide-field monitoring of the dynamic radio sky ...
Dodson, R., Deshpande, A., Lewis, D., McCulloch, P.   +3 more
openaire   +2 more sources

The Birthplaces of Pulsars [PDF]

Symposium - International Astronomical Union, 1974
With the refinement of the estimates of electron density in the Galaxy it is clear that pulsars have z distances away from the galactic plane of a few hundred parsec. There is now a very strong indication that young pulsars lie at small z distances, suggesting that pulsars originate in a small z population and are given velocities of about 100 km s-1 ...
openaire   +2 more sources

A Study on the Evolution of Emission Altitude with Frequency Among 104 Normal Pulsars

Universe
Utilizing the databases from the European Pulsar Network (EPN), the Australia Telescope National Facility (ATNF), and published literature data, a geometric method was used to investigate the multifrequency emission altitude of 104 pulsars. We found that
Chaoxin Luo, Xin Xu, Changrong Du, Qijun Zhi   +3 more
doaj   +1 more source

The strongest magnetic fields in the universe: How strong can they become?

Frontiers in Physics, 2014
Magnetic fields in the universe are in general weak, of the order of µGauss only. However, in compact objects they assume extraordinarily large values. These are produced by gravitational collapse of massive magnetised objects.
Rudolf A. Treumann, Wolfgang eBaumjohann, André eBalogh   +2 more
doaj   +1 more source

On Period and Burst Histories of AXPs and SGRs and the Possible Evolution of these Objects on the P-Pdot Diagram

, 2002
In this paper, timing data for all of the anomalous X-ray pulsars and soft gamma repeaters are compiled. Timing properties of these objects are investigated. The effect of bursts of soft gamma repeaters on their period history is investigated. The P-Pdot
Ankay, Askin, Guseinov, Oktay H., Tagieva, Sevinc, Yazgan, Efe   +3 more
core   +1 more source

On H II Regions and Pulsar Distances* [PDF]

, 1969
A. J. R. Prentice, D. ter Haar
openalex   +1 more source

Rotating Quark Stars in General Relativity

Universe, 2018
We have built quasi-equilibrium models for uniformly rotating quark stars in general relativity. The conformal flatness approximation is employed and the Compact Object CALculator (cocal) code is extended to treat rotating stars with surface density ...
Enping Zhou, Antonios Tsokaros, Luciano Rezzolla, Renxin Xu, Kōji Uryū   +4 more
doaj   +1 more source

A Search for Pulsed Gamma Emission from Two Pulsars [PDF]

, 1969
J. G. Ables, J. M. Durdin, A. G. Gregory, B.J. Stone   +3 more
openalex   +1 more source