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Journal Article PUBDB-2025-00833

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Diffuse continuum emission and large extended sources at MeV energies

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2025
Reidel Dordrecht

Space science reviews 221(7), 92 () [10.1007/s11214-025-01215-0]
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Report No.: arXiv:2510.07311

Abstract: Future gamma-ray survey instruments, such as newASTROGAM and AMEGO-X, willsignificantly improve previous and current all-sky surveys at MeV energies. Inthis paper we discuss the continuum emission from the Milky Way, two prominentlarge extended sources, the Fermi bubbles and Loop I, and the extragalacticgamma-ray background. We highlight the importance of measurements in the MeV toGeV energy range for understanding CR production and propagation in the Galaxy,for the determination of the nature of the Fermi bubbles and Loop I, and forexploring the origin of the extragalactic gamma-ray background.

Classification:

Note: 27 pages, 5 figures, part of the 'Unveiling the MeV Universe in the Multi-Messenger Era' collection in Space Science Reviews

Contributing Institute(s):
  1. Gammaastronomie (Z_GA)
  2. Neutrinoastronomie / Kosmologie (Z_NA)
Research Program(s):
  1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2025
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Medline ; Clarivate Analytics Master Journal List ; Current Contents - Physical, Chemical and Earth Sciences ; DEAL Springer ; DEAL Springer ; Ebsco Academic Search ; Essential Science Indicators ; IF >= 10 ; JCR ; SCOPUS ; Science Citation Index Expanded ; Web of Science Core Collection
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Diffuse Continuum Emission and Large Extended Sources at MeV Energies
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 Record created 2025-02-26, last modified 2025-11-19