Results 171 to 180 of about 654,536 (207)
An interstellar mission to test astrophysical black holes. [PDF]
Bambi C.
europepmc +1 more source
<i>NICER</i> and <i>Fermi</i> GBM Observations of the First Galactic Ultraluminous X-ray Pulsar Swift J0243.6+6124. [PDF]
Wilson-Hodge CA +21 more
europepmc +1 more source
Multiwavelength constraints on the origin of a nearby repeating fast radio burst source in a globular cluster. [PDF]
Pearlman AB +28 more
europepmc +1 more source
Fast radio bursts and the radio perspective on multi-messenger gravitational lensing. [PDF]
Pastor-Marazuela I.
europepmc +1 more source
Electromagnetic follow-up of gravitational waves: review and lessons learned. [PDF]
Nicholl M, Andreoni I.
europepmc +1 more source
Comparing human vs. machine-assisted analysis to develop a new approach for Big Qualitative Data Analysis. [PDF]
Martin S +10 more
europepmc +1 more source
Binary and Millisecond Pulsars [PDF]
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.
Shrinivas Kulkarni, Edward Sterl Phinney
exaly +6 more sources
Populating the Galaxy With Pulsars I. Stellar and Binary Evolution
The computation of theoretical pulsar populations has been a major component of pulsar studies since the 1970s.However, the majority of pulsar population synthesis has only regarded isolated pulsar evolution.
Jarrod Robert Hurley, Matthew Bailes
exaly +2 more sources

