Results 141 to 150 of about 1,910,738 (272)

Hadronic model for radio-to-TeV gamma-ray emission from PSR B1259-63

open access: yes, 2006
We discuss the implications of the recent X-ray and TeV gamma-ray observations of the PSR B1259-63 system (a young rotation powered pulsar orbiting a Be star) for the theoretical models of interaction of pulsar and stellar winds.
Andrii Neronov   +12 more
core   +1 more source

Magnetic Field Geometry of the Gamma-Ray Binary PSR B1259–63 Revealed via X-Ray Polarization

open access: yesThe Astrophysical Journal Letters
Some X-ray binaries containing an energetic pulsar in orbit around a normal star accelerate particles to high energies in the shock cone formed where the pulsar and stellar winds collide.
Philip Kaaret   +8 more
doaj   +1 more source

The Zoo of X-ray Pulsars

open access: yes, 2001
12 pages, latex, 1 figure, 2 tables Contains an updated list of X-ray pulsars in the Magellanic Clouds. Invited Talk presented at the Workshop Frontier Objects in Astrophysics and Particle Physics, Vulcano (Italy), May 22-27 ...
openaire   +2 more sources

An X-Ray Synchrotron Shell and a Pulsar: The Peculiar Supernova Remnant G32.4+0.1

open access: yesThe Astrophysical Journal
We present a deep Chandra observation of the shell supernova remnant (SNR) G32.4+0.1, whose featureless X-ray spectrum has led to its classification as an X-ray synchrotron-dominated SNR. We find a partial shell morphology whose outline is quite circular,
Stephen P. Reynolds   +1 more
doaj   +1 more source

Discovery of Diffuse Hard X-Ray Emission from the Vicinity of PSR J1648-4611 with Suzaku

open access: yes, 2013
We observed the pulsar PSR J1648-4611 with Suzaku. Two X-ray sources, Suzaku J1648-4610 (Src A) and Suzaku J1648-4615 (Src B), were found in the field of view. Src A is coincident with the pulsar PSR J1648-4611, which was also detected by the Fermi Gamma-
Haba, Yoshito   +4 more
core   +1 more source

Intermittent stellar wind accretion and the long-term activity of Population I binary systems containing an X-ray pulsar

open access: yes, 1986
On compare les proprietes observees des binaires de population I contenant des pulsars RX avec differents regimes d'accretion par vent a l'interieur d'une etoile a neutrons ...
L. Stella, N. White, R. Rosner
semanticscholar   +1 more source

Optical candidates for two X-ray bursters and an X-ray pulsar [PDF]

open access: green, 1977
J. E. McClintock   +5 more
openalex   +1 more source

The transient 42 second X-ray pulsar EXO 2030+375. II: The luminosity dependence of the pulse profile

open access: yes, 1989
During an outburst from the transient, 42 s, X-ray pulsar EXO 2030+375, marked luminosity-dependent changes in pulsar profile were observed. At high luminosities the pulse profile consisted of a smooth asymmetric main pulse separated by about 180 deg in ...
A. Parmar, N. White, L. Stella
semanticscholar   +1 more source

XMM-Newton observation of PSR B2224+65 and its jet

open access: yes, 2011
We have investigated the pulsar PSR B2224+65 and its X-ray jet with XMM-Newton. Apart from the long X-ray jet which is almost perpendicular to the direction of proper motion, a putative extended feature at the pulsar position, which oriented in the ...
Abdo   +35 more
core   +1 more source

A possible association of the new VHE gamma-ray source HESS J1825--137 with the pulsar wind nebula G18.0--0.7

open access: yes, 2005
We report on a possible association of the recently discovered very high-energy $\gamma$-ray source HESS J1825--137 with the pulsar wind nebula (commonly referred to as G 18.0--0.7) of the $2.1\times 10^{4}$ year old Vela-like pulsar PSR B1823--13.
A. Djannati-Ataï   +114 more
core   +2 more sources

Home - About - Disclaimer - Privacy