van Eldik C (2008)
Publication Status: Published
Publication Type: Journal article, Original article
Publication year: 2008
Publisher: Elsevier
Book Volume: 588
Pages Range: 72-75
DOI: 10.1016/j.nima.2008.01.025
Measurements by High Energy Stereoscopic System (H.E.S.S.) provide the first sensitive map of very-high-energy (VHE) γ-ray emission from the central few hundred parsecs of our galaxy. These observations are a valuable tool to understand the acceleration and propagation of energetic particles near the Galactic Centre (GC). The data reveal the existence of three discrete VHE γ-ray sources and the presence of diffuse γ-ray emission correlated with dense molecular clouds. The H.E.S.S. view of the GC region is reviewed, and possible counterparts of H.E.S.S. sources are discussed. © 2008 Elsevier B.V. All rights reserved.
APA:
van Eldik, C. (2008). The H.E.S.S. view of the Galactic Centre region. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 588, 72-75. https://doi.org/10.1016/j.nima.2008.01.025
MLA:
van Eldik, Christopher. "The H.E.S.S. view of the Galactic Centre region." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 588 (2008): 72-75.
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