Results 141 to 150 of about 34,678 (162)

Multiwavelength constraints on the origin of a nearby repeating fast radio burst source in a globular cluster. [PDF]

Nat Astron
Pearlman AB, Scholz P, Bethapudi S, Hessels JWT, Kaspi VM, Kirsten F, Nimmo K, Spitler LG, Fonseca E, Meyers BW, Stairs IH, Tan CM, Bhardwaj M, Chatterjee S, Cook AM, Curtin AP, Dong FA, Eftekhari T, Gaensler BM, Güver T, Kaczmarek J, Leung C, Masui KW, Michilli D, Prince TA, Sand KR, Shin K, Smith KM, Tendulkar SP.   +28 more
europepmc   +1 more source

Ultra high energy electrons powered by pulsar rotation. [PDF]

Sci Rep, 2013
Mahajan S, Machabeli G, Osmanov Z, Chkheidze N.   +3 more
europepmc   +1 more source

Foreword to the special issue commemorating Volume 100 of Science Progress. [PDF]

Sci Prog, 2017
Phillips D.
europepmc   +1 more source

Monte Carlo Modeling of An Experimental Benchtop L-shell X-ray Fluorescence Imaging/CT System Adopting Two Silicone Drift Detectors. [PDF]

Nucl Instrum Methods Phys Res A
Nepal N, Kaphle A, Jayarathna S, Cho SH.
europepmc   +1 more source

The orbital dynamics of the LMC and SMC about the Milky Way. [PDF]

Astron Astrophys Rev
Besla G, Kallivayalil N.
europepmc   +1 more source

Gravitational waves from dark domain walls

Christiansen Ø, Adamek J, Hassani F, Mota DF.   +3 more
europepmc   +1 more source

Gamma rays from millisecond pulsars [PDF]

Journal of Astrophysics and Astronomy, 1991
The contribution of millisecond pulsars to the diffuse gamma-ray background of the Galaxy is estimated, and it is shown that a significant fraction of the Galactic background may originate from them. A small number of the unidentified COS-B point sources
Dipankar Bhattacharya
exaly   +2 more sources

Polarization observations of 20 millisecond pulsars [PDF]

Monthly Notices of the Royal Astronomical Society, 2011
Polarization profiles are presented for 20 millisecond pulsars that are being observed as part of the Parkes Pulsar Timing Array project. The observations used the Parkes multibeam receiver with a central frequency of 1369 MHz and the Parkes digital ...
Aidan W Hotan, Richard Manchester, Joris Verbiest   +2 more
exaly   +4 more sources

The minimum rotation period of millisecond pulsars

Monthly Notices of the Royal Astronomical Society: Letters, 2021
A simple and natural explanation for the minimum period of millisecond pulsars follows from a correlation between the accretion rate and the frozen surface dipole magnetic field resulting from ohmic diffusion through the neutron star crust in initial ...
Mehmet Ali Alpar, Ünal Ertan
exaly   +2 more sources