Results 111 to 120 of about 120,893 (256)
Search for a Correlation Between Radio Giant Pulses and VHE Photons of the Crab Pulsar
The Crab pulsar is a unique source of pulsar radio emission. Its regular pulse structure is visible over the entire electromagnetic spectrum from radio to GeV ranges.
N. Lewandowska+2 more
doaj
Anticorrelation Between Flux and Photon Index of Hard-X-Ray Emission from the Crab
Using Swift Burst Alert Telescope event-mode data during gamma-ray burst occurrences, we conduct spectral analysis for the Crab system. From 38 good observations, which span a period of 18 yr from 2006 to 2023, we find that the Crab’s X-ray flux not only
Koothodil Abhijith Augustine+1 more
doaj +1 more source
Synchrotron Pair Production Equilibrium in Relativistic Magnetic Reconnection
Magnetic reconnection is ubiquitous in astrophysical systems, and in many such systems the plasma suffers from significant cooling due to synchrotron radiation.
Alexander Y. Chen+2 more
doaj +1 more source
EVOLUTION OF THE X-RAY PROFILE OF THE CRAB PULSAR [PDF]
Using the archival data from the Rossi X-ray Timing Explorer, we study the evolution of the Crab pulsar’s X-ray profile in a time span of 11 years. The X-ray profiles, as characterized by a few parameters, changed slightly, but with high statistical ...
M. Ge+7 more
semanticscholar +1 more source
The supernova remnant (SNR) 0540–69.3, twin of the Crab Nebula, offers an excellent opportunity to study the continuum emission from a young pulsar and pulsar wind nebula (PWN). We present observations taken with the Very Large Telescope instruments MUSE
L. Tenhu+6 more
doaj +1 more source
THE CRAB PULSAR AT CENTIMETER WAVELENGTHS. I. ENSEMBLE CHARACTERISTICS [PDF]
We have observed the pulsar in the Crab Nebula at high radio frequencies and high time resolution. We present continuously sampled data at 640 ns time resolution and individual bright pulses recorded at down to 0.25 ns time resolution.
T. Hankins, Glenn Jones, J. Eilek
semanticscholar +1 more source
Polarimetric Evidence of the First White Dwarf Pulsar: The Binary System AR Scorpii
The binary star AR Scorpii was recently discovered to exhibit high amplitude coherent variability across the electromagnetic spectrum (ultraviolet to radio) at two closely spaced ∼2 min periods, attributed to the spin period of a white dwarf and the beat
David A.H. Buckley+4 more
doaj +1 more source
The present generation of Imaging Air Cherenkov Telescopes (IACTs) has greatly improved our knowledge on the Very High Energy (VHE) side of our Universe. The MAGIC IACTs operate since 2004 with one telescope and since 2009 as a two telescope stereoscopic
López-Coto Rubén
doaj +1 more source
Galactic PeV cosmic-ray accelerators (PeVatrons) are Galactic sources theorized to accelerate cosmic rays up to PeV in energy. The accelerated cosmic rays are expected to interact hadronically with nearby ambient gas or the interstellar medium, resulting
R. Abbasi+389 more
doaj +1 more source
On scattering of Giant Pulses from the Crab Pulsar: a Scattering Function [PDF]
Simultaneous dual-frequency observations of giant pulses from the Crab pulsar were performed at the frequencies of 61 and 111 MHz. It is shown that scattering of giant pulses from the Crab pulsar occurs at thick, and not at thin screen.
arxiv