Results 171 to 180 of about 3,309 (210)

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

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

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

Hyperons: the strange ingredients of the nuclear equation of state. [PDF]

Proc Math Phys Eng Sci, 2018
Vidaña I.
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 Confrontation between General Relativity and Experiment. [PDF]

Living Rev Relativ, 2014
Will CM.
europepmc   +1 more source

Gravitational waves from dark domain walls

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

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Millisecond Pulsars

2022
Andrew Lyne, Francis Graham-Smith, Benjamin Stappers   +2 more
exaly   +3 more sources

Binary and Millisecond Pulsars [PDF]

Annual Review of Astronomy and Astrophysics, 1994
Most of the ~600 known pulsars are single and located in the disk of our Galaxy. There is circumstantial evidence that the pulsars in this majority are created in supernova (SN) explosions, by the collapse of the cores of massive stars (initial mass M_i ≳ M_(cr) ≃ 8 M_⊙). One is created roughly every 100 y in the Galaxy.
E S Phinney, S R Kulkarni
exaly   +4 more sources

A millisecond pulsar

Nature, 1982
The radio properties of 4C21.53 have been an enigma for many years. First, the object displays interplanetary scintillations (IPS) at 81 MHz, indicating structure smaller than 1 are s, despite its low galactic latitude (−0.3°)1. IPS modulation is rare at low latitudes because of interstellar angular broadening. Second, the source has an extremely steep
Backer, D. C., Kulkarni, Shrinivas R., Heiles, Carl, Davis, M. M., Goss, W. M.   +4 more
openaire   +2 more sources