Pulsar wind nebulae in supernova remnants [PDF]
E. van der Swaluw+3 more
openalex +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
A GeV-TeV particle component and the barrier of cosmic-ray sea in the Central Molecular Zone. [PDF]
Huang X, Yuan Q, Fan YZ.
europepmc +1 more source
Magnetic fields and relativistic electrons fill entire galaxy cluster. [PDF]
Botteon A+15 more
europepmc +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
Analysis of Crab X-Ray Polarization Using Deeper Imaging X-Ray Polarimetry Explorer Observations
We present Crab X-ray polarization measurements using Imaging X-Ray Polarimetry Explorer (IXPE) data with a total exposure of 300 ks, three times more than the initial 2022 discovery paper.
Josephine Wong+100 more
doaj +1 more source
Correlation between the X-ray Spectra of Young Pulsars and their Wind Nebulae [PDF]
E. V. Gotthelf
openalex +1 more source
The GeV γ-Ray Emission from the Composite Supernova Remnant CTB 87
We report the GeV γ -ray emission around the composite supernova remnant (SNR) CTB 87 with more than 16 yr of PASS 8 data recorded by the Fermi Large Area Telescope. Two separate point sources with different GeV spectra are identified in this region: one
Yuliang Xin+5 more
doaj +1 more source
Discovering the sky at the longest wavelengths with a lunar orbit array. [PDF]
Chen X+6 more
europepmc +1 more source
X‐Ray Spectra of Young Pulsars and Their Wind Nebulae: Dependence on Spin‐Down Energy Loss Rate [PDF]
E. V. Gotthelf
openalex +1 more source