Results 21 to 30 of about 43,788 (263)
Mission Overview and Initial Observation Results of the X-Ray Pulsar Navigation-I Satellite
International Journal of Aerospace Engineering, 2017 The newly launched X-ray pulsar navigation-I (XPNAV-1) is an experimental satellite of China that is designed for X-ray pulsar observation. This paper presents the initial observation results and aims to recover the Crab pulsar’s pulse profile to verify ...
Xinyuan Zhang +4 more
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Novel X-ray Communication Based XNAV Augmentation Method Using X-ray Detectors
Sensors, 2015 The further development of X-ray pulsar-based NAVigation (XNAV) is hindered by its lack of accuracy, so accuracy improvement has become a critical issue for XNAV.
Shibin Song +3 more
doaj +1 more source
Frontiers in Materials, 2021 An X-ray pulsar is a remnant of massive star evolution, collapse, and supernova explosions. It has an extremely stable spin cycle and is known as the most accurate astronomical clock in the natural world.
Manwen Liu +9 more
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Accretion onto Fast X‐Ray Pulsars
The Astrophysical Journal, 2004 10 pages, 5 figures, submitted to ...
Rappaport, S., Fregeau, J., Spruit, H.
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Accretion powered X-ray pulsars [PDF]
The Astrophysical Journal, 1983 A unified description of the properties of 14 X-ray pulsars is presented and compared with the current theoretical understanding of these systems. The sample extends over six orders of magnitude in luminosity, with the only trend in the phase averaged spectra being that the lower luminosity systems appear to have less abrupt high energy cutoffs.
N. E. White, J. H. Swank, S. S. Holt
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Chandra observations of the pulsar wind nebula in SNR G0.9+0.1 [PDF]
, 2001 We present observations with the Chandra X-ray Observatory of the pulsar wind nebula (PWN) within the supernova remnant G0.9+0.1. At Chandra's high resolution, the PWN has a clear axial symmetry; a faint X-ray point source lying along the symmetry axis ...
B. M. Gaensler +10 more
core +2 more sources
The Astrophysical Journal, 2023 We report on the X-ray emission properties of the pulsar PSR J1849−0001 and its wind nebula (PWN), as measured by Chandra, XMM-Newton, NICER, Swift, and NuSTAR.
Chanho Kim +8 more
doaj +1 more source
Nuclear Physics B - Proceedings Supplements, 2004 We review the observational properties of the class of young neutron stars known as "anomalous X-ray pulsars," emphasizing the tremendous progress that has been made in recent years, and explain why these objects, like the "soft gamma repeaters," are today thought to be young, isolated, ultrahigh magnetic field neutron stars, or "magnetars."
Kaspi, V. M., Gavriil, F. P.
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Studying millisecond pulsars in X-rays [PDF]
Astrophysics and Space Science, 2007 To appear in Astrophysics and Space Science, Proceedings of "Isolated Neutron Stars: from the Interior to the Surface", eds. D. Page, R. Turolla and S.
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Multi-wavelength observations of 2HWC J1928+177: dark accelerator or new TeV gamma-ray binary?
, 2020 2HWC J1928+177 is a Galactic TeV gamma-ray source detected by the High Altitude Water Cherenkov (HAWC) Observatory up to ~ 56 TeV. The HAWC source, later confirmed by H.E.S.S., still remains unidentified as a dark accelerator since there is no apparent ...
An, Hongjun +11 more
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