Results 161 to 170 of about 11,249 (249)

The GeV γ-Ray Emission from the Composite Supernova Remnant CTB 87

The Astrophysical Journal
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, Jian Tang, Weixiong Ding, Xi Liu, Yunfeng Zhang, Xiaolei Guo   +5 more
doaj   +1 more source

Discovering the sky at the longest wavelengths with a lunar orbit array. [PDF]

Philos Trans A Math Phys Eng Sci, 2021
Chen X, Yan J, Deng L, Wu F, Wu L, Xu Y, Zhou L.   +6 more
europepmc   +1 more source

X‐Ray Spectra of Young Pulsars and Their Wind Nebulae: Dependence on Spin‐Down Energy Loss Rate [PDF]

, 2003
E. V. Gotthelf
openalex   +1 more source

Constraining Anisotropic Diffusion between Geminga and Earth with the Cosmic-Ray Electron and Positron Spectrum

The Astrophysical Journal
The gamma-ray halo around Geminga indicates significant suppression of cosmic-ray diffusion. One possible explanation for this phenomenon is the projection effect of slow diffusion perpendicular to the mean magnetic field (characterized by the diffusion ...
Junji Xia, Xiaojun Bi, Kun Fang, Siming Liu   +3 more
doaj   +1 more source

Spherically symmetric relativistic MHD simulations of pulsar wind nebulae in supernova remnants [PDF]

, 2003
N. Bucciantini, John M. Blondin, L. Del Zanna, Elena Amato   +3 more
openalex   +1 more source

Study of Magnetic Field and Turbulence in the TeV Halo around the Monogem Pulsar

The Astrophysical Journal
Magnetic fields are ubiquitous in the interstellar medium, including extended objects such as supernova remnants and diffuse halos around pulsars. Its turbulent characteristics govern the diffusion of cosmic rays and the multiwavelength emission from ...
Sunil Malik, Ka Ho Yuen, Huirong Yan
doaj   +1 more source

Correlation between the X-ray Spectra of Young Pulsars and their Wind Nebulae [PDF]

, 2003
E. V. Gotthelf
openalex   +1 more source

Spatial Variations and Breaks in the Optical–Near-infrared Spectra of the Pulsar and Pulsar Wind Nebula in Supernova Remnant 0540–69.3

The Astrophysical Journal
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, J. Larsson, J. Sollerman, P. Lundqvist, J. Spyromilio, J. D. Lyman, G. Olofsson   +6 more
doaj   +1 more source

How unique are pulsar wind nebulae models? Implementation of a multi-parameter, automatic fitting for time-dependent spectra [PDF]

Journal of High Energy Astrophysics, 2022
J. Martin, D. Torres
semanticscholar   +1 more source

Millimeter-wave Imaging of Pulsar Wind Nebulae [PDF]

, 2004
D. C.‐J. Bock, B. M. Gaensler
openalex   +1 more source