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HESS Observations of the Galactic Center Region and Their Possible Dark Matter Interpretation
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Link:
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Erscheinungsjahr:
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2006
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Medientyp:
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Text
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Schlagworte:
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98.70.Rz
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95.35.+d
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95.85.Pw
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98.35.Jk
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gamma-ray sources
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gamma-ray bursts
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Dark matter
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gamma-ray
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Galactic center bar circumnuclear matter and bulge
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Astrophysics
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Beschreibung:
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The detection of γ rays from the source HESS J1745-290 in the Galactic Center (GC) region with the High Energy Spectroscopic System (HESS) array of Cherenkov telescopes in 2004 is presented. After subtraction of the diffuse γ-ray emission from the GC ridge, the source is compatible with a point source with spatial extent less than 1.2′(stat) (95% C.L.). The measured energy spectrum above 160 GeV is compatible with a power law with photon index of 2.25±0.04(stat)±0.10(syst) and no significant flux variation is detected. It is finally found that the bulk of the very high energy emission must have non-dark-matter origin. © 2006 The American Physical Society.
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Lizenz:
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info:eu-repo/semantics/restrictedAccess
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Quellsystem:
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Forschungsinformationssystem der UHH
Interne Metadaten
- Quelldatensatz
- oai:www.edit.fis.uni-hamburg.de:publications/a24c5d72-edda-48b1-a720-0df488352521