Superfluid Spin-up: Three-dimensional Simulations of Post-glitch Dynamics in Neutron Star Cores
Neutron stars show a steady decrease in their rotational frequency, occasionally interrupted by sudden spin-up events called glitches. The dynamics of a neutron star after a glitch involve the transfer of angular momentum from the crust (where the glitch
J. R. Fuentes, Vanessa Graber
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The high energy X-ray probe (HEX-P): magnetars and other isolated neutron stars
The hard X-ray emission from magnetars and other isolated neutron stars remains under-explored. An instrument with higher sensitivity to hard X-rays is critical to understanding the physics of neutron star magnetospheres and also the relationship between
J. A. J. Alford +27 more
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Auroral emissions from Uranus and Neptune. [PDF]
Lamy L.
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Limits to Extracting Neutron-star Physics Constraints from NICER Pulse Profiles
Modeling energy-dependent X-ray pulse profiles from rotation-powered millisecond pulsars observed with Neutron Star Interior and Composition Explorer (NICER) has emerged as a promising avenue for measuring neutron-star radii and probing the equation of ...
Tolga Güver +3 more
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On the Coupling of Rotation Powered Pulsars to Plerionic Nebulae
19 pages, 3 figures, to be published in Mem. Soc. Ast.
openaire +2 more sources
Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical impact of cosmic rays. [PDF]
Ruszkowski M, Pfrommer C.
europepmc +1 more source
Magnetohydrodynamic simulations of binary neutron star mergers in general relativity: Effects of magnetic field orientation on jet launching. [PDF]
Ruiz M, Tsokaros A, Shapiro SL.
europepmc +1 more source
X-ray studies of neutron stars and their magnetic fields. [PDF]
Makishima K.
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