Results 1 to 10 of about 155 (144)
Ultra high energy electrons powered by pulsar rotation. [PDF]
Sci Rep, 2013 12 pages, 3 ...
Mahajan S +3 more
europepmc +5 more sources
Glitches and Glitching Clusters in Rotation-powered Pulsars
The Astrophysical JournalThe study of pulsar glitch phenomena serves as a valuable probe into the dynamic properties of matter under extreme high-density conditions, offering insights into the physics within neutron stars.
Pei-Xin Zhu, Xiao-Ping Zheng
doaj +3 more sources
CONSTRAINING RELATIVISTIC BOW SHOCK PROPERTIES IN ROTATION-POWERED MILLISECOND PULSAR BINARIES. [PDF]
Astrophys J, 2017 Accepted to ApJ, 36 pages, 15 figures; comments ...
Wadiasingh Z +4 more
europepmc +5 more sources
A New X-Ray Census of Rotation Powered Pulsars
The Astrophysical JournalTo date, over 4000 pulsars have been detected. In this study, we identify 231 X-ray counterparts of Australia Telescope National Facility (ATNF) pulsars by performing a spatial cross match across the Chandra, XMM-Newton observational catalogs.
Yu-Jing Xu +4 more
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Multiwavelength Polarization of Rotation-powered Pulsars [PDF]
The Astrophysical Journal, 2017 Abstract Polarization measurements provide strong constraints on models for emission from rotation-powered pulsars. We present multiwavelength polarization predictions showing that measurements over a range of frequencies can be particularly important for constraining the emission location, radiation mechanisms, and system geometry.
Alice K. Harding +1 more
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Polarization Sweeps in Rotation‐powered Pulsars [PDF]
The Astrophysical Journal, 2001 23 pages, 8 figures; accepted by ...
Hibschman, Johann A., Arons, Jonathan
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High Magnetic Field Rotation-powered Pulsars [PDF]
AIP Conference Proceedings, 2011 6 pages, 4 figures, Conference proceeding of "ASTROphysics of Neutron Stars 2010 -- a conference in honor of M.
C.-Y. Ng +4 more
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Green Bank Telescope Discovery of the Redback Binary Millisecond Pulsar PSR J0212+5321
The Astrophysical Journal, 2023 We report the discovery of a 2.11 ms binary millisecond pulsar during a targeted search of the redback optical candidate coincident with the γ -ray source 3FGL J0212.5+5320 using the Robert C.
Karen I. Perez +3 more
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On the angular momentum extraction from the rotation powered pulsars [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 ABSTRACT The rotation powered pulsar loses angular momentum at a rate of the rotation power divided by the angular velocity Ω*. This means that the length of the lever arm of the angular momentum extracted by the photons, relativistic particles, and wind must be on average c/Ω*, which is known as the light cylinder radius. Therefore, any
Shibata, Shinpei, Kisaka, Shota
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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
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