Constraints on the e± pair injection of pulsar halos: Implications from the Galactic diffuse multi-TeV gamma-ray emission
Author:
Funder
National Natural Science Foundation of China
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.107.103028/fulltext
Reference49 articles.
1. FERMI-LAT OBSERVATIONS OF THE DIFFUSE γ-RAY EMISSION: IMPLICATIONS FOR COSMIC RAYS AND THE INTERSTELLAR MEDIUM
2. Galactic diffuse gamma-ray emission at TeV energy
3. Evidence for TeV Gamma-Ray Emission from a Region of the Galactic Plane
4. STUDY OF THE DIFFUSE GAMMA-RAY EMISSION FROM THE GALACTIC PLANE WITH ARGO-YBJ
5. First Detection of sub-PeV Diffuse Gamma Rays from the Galactic Disk: Evidence for Ubiquitous Galactic Cosmic Rays beyond PeV Energies
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1. Diffuse ultrahigh-energy gamma-ray emission from TeV halos;Physical Review D;2024-04-22
2. Insights from LHAASO and IceCube into the origin of the Galactic diffuse teraelectronvolt–petaelectronvolt emission;Nature Astronomy;2024-03-13
3. Could the TeV emission of starburst galaxies originate from pulsar wind nebulae?;Monthly Notices of the Royal Astronomical Society;2023-11-27
4. Galactic Diffuse γ-Ray Emission from GeV to PeV Energies in Light of Up-to-date Cosmic-Ray Measurements;The Astrophysical Journal;2023-10-26
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