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- Lawrence Berkeley National LaboratoryUS223 papers
- Centre National de la Recherche ScientifiqueFR218 papers
- University of MichiganUS186 papers
- Fermi National Accelerator LaboratoryUS182 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR182 papers
- University of ManchesterGB182 papers
- Michigan State UniversityUS179 papers
- University of California, BerkeleyUS179 papers
- Sorbonne UniversitéFR178 papers
- Joint Institute for Nuclear ResearchRU174 papers
- Iowa State UniversityUS173 papers
- Columbia UniversityUS171 papers
5 papers · 2 filters
Accretion-powered pulsations in an apparently quiescent neutron star binary
Anne M. Archibald, Slavko Bogdanov, Alessandro Patruno +10
Accreting millisecond X-ray pulsars are an important subset of low-mass X-ray binaries in which coherent X-ray pulsations can be observed during occasional, bright outbursts (X-ray…
Green Bank Telescope and Swift X-ray Telescope Observations of the Galactic Center Radio Magnetar SGR J1745-2900
Ryan S. Lynch, Robert F. Archibald, Victoria M. Kaspi +1
We present results from eight months of Green Bank Telescope 8.7-GHz observations and nearly 18 months Swift X-ray telescope observations of the radio magnetar SGR J1745-2900, whic…
An Ultraluminous X-ray Source Powered by An Accreting Neutron Star
M. Bachetti, F. A. Harrison, D. J. Walton +21
Ultraluminous X-ray sources (ULX) are off-nuclear point sources in nearby galaxies whose X-ray luminosity exceeds the theoretical maximum for spherical infall (the Eddington limit)…
Disordered nuclear pasta, magnetic field decay, and crust cooling in neutron stars
C. J. Horowitz, D. K. Berry, C. M. Briggs +3
Nuclear pasta, with non-spherical shapes, is expected near the base of the crust in neutron stars. Large scale molecular dynamics simulations of pasta show long lived topological d…
NuSTAR Observations of the Magnetar 1E 2259+586
Julia K. Vogel, Romain Hascoet, Victoria M. Kaspi +15
We report on new broad band spectral and temporal observations of the magnetar 1E 2259+586, which is located in the supernova remnant CTB 109. Our data were obtained simultaneously…