HESS J1826-130

  • HESS J1826-130 is an unidentified hard spectrum source discovered by H.E.S.S. along the Galactic plane, the spectral index being Gamma = 1.6 with an exponential cut-off at about 12 TeV. While the source does not have a clear counterpart at longer wavelengths, the very hard spectrum emission at TeV energies implies that electrons or protons accelerated up to several hundreds of TeV are responsible for the emission. In the hadronic case, the VHE emission can be produced by runaway cosmic-rays colliding with the dense molecular clouds spatially coincident with the H.E.S.S. source.

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Metadaten
Author details:Ekrem Oǧuzhan AngünerGND, Felix A. AharonianORCiDGND, Pol BordasORCiDGND, Sabrina CasanovaGND, Clemens HoischenORCiDGND, I. Oya, A. Ziegler
DOI:https://doi.org/10.1063/1.4968928
ISBN:978-0-7354-1456-3
ISSN:0094-243X
ISSN:1551-7616
Title of parent work (English):AIP conference proceedings / American Institute of Physics
Subtitle (English):a very hard gamma-Ray spectrum source in the Galactic Plane
Publisher:American Institute of Physics
Place of publishing:Melville
Publication type:Other
Language:English
Date of first publication:2017/01/04
Publication year:2017
Creating corporation:HESS Collaboration
Release date:2022/11/24
Volume:1792
Issue:1
Number of pages:6
Organizational units:Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie
DDC classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Peer review:Referiert
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