Results 71 to 80 of about 47,603 (141)
Spatially Resolved Polarization Variation of the Crab Nebula
We examined the spatially resolved polarization variations in the Crab Nebula over 2 yr, using observational data from the Imaging X-ray Polarimetry Explorer, and offer key insights into its magnetic field structures and evolution.
Chao Zuo+8 more
doaj +1 more source
Multiwavelength Observations of Pulsar Wind Nebulae [PDF]
The extended nebulae formed as pulsar winds expand into their surroundings provide information about the composition of the winds, the injection history from the host pulsar, and the material into which the nebulae are expanding. Observations from across the electromagnetic spectrum provide constraints on the evolution of the nebulae, the density and ...
arxiv +1 more source
The ultra-high-energy (UHE) Galactic diffuse gamma-ray emission holds important information on the propagation of cosmic rays in the Galaxy. However, its measurements suffer from a contamination from unresolved sources whose contribution remains unclear.
Samy Kaci+2 more
doaj +1 more source
This paper investigates the origin of the γ -ray emission from MGRO J1908+06 in the GeV–TeV energy band. By analyzing the data collected by the Fermi Large Area Telescope, the Very Energetic Radiation Imaging Telescope Array System, and High Altitude ...
A. Acharyya+129 more
doaj +1 more source
Observations of Supernova Remnants and Pulsar Wind Nebulae: A VERITAS Key Science Project [PDF]
The study of supernova remnants and pulsar wind nebulae was one of the Key Science Projects for the first two years of VERITAS observations. VERITAS is an array of four imaging Cherenkov telescopes located at the Whipple Observatory in southern Arizona. Supernova remnants are widely considered to be the strongest candidate for the source of cosmic rays
arxiv
A Catalog of Pulsar X-Ray Filaments
We present the first Chandra X-ray Observatory (CXO) catalog of “pulsar X-ray filaments,” or “misaligned outflows.” These are linear, synchrotron-radiating features powered by ultrarelativistic electrons and positrons that escape from bow shock pulsars ...
Jack T. Dinsmore, Roger W. Romani
doaj +1 more source
Unraveling the Nature of HAWC J1844–034 with Fermi-LAT Data Analysis and Multiwavelength Modeling
The extended ultra-high-energy (UHE) gamma-ray source HAWC J1844–034 is closely associated with two other sources, HAWC J1843–032 and HWC J1846–025. Moreover, other gamma-ray observatories like HESS, LHAASO, and Tibet AS _γ have detected UHE gamma-ray ...
Sovan Boxi+2 more
doaj +1 more source
Pulsar Wind Nebulae in Evolved Supernova Remnants [PDF]
John M. Blondin+2 more
openalex +1 more source
Pulsar wind nebulae in supernova remnants [PDF]
E. van der Swaluw+3 more
openalex +1 more source
A Cacophony of Echoes from Daily Monitoring of the Crab Pulsar at Jodrell Bank
Using archival data from the 42-foot telescope at the Jodrell Bank Observatory, we produce daily stacks of aligned giant pulses for the Crab pulsar, to study changes to the daily profiles between 2012 April and 2016 December.
Thierry Serafin Nadeau+5 more
doaj +1 more source