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Detection of very high energy radiation from HESS J1908+063 confirms the Milagro unidentified source MGRO J1908+06
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- Autor/in:
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- Aharonian, F.
- Akhperjanian, A. G.
- Anton, G.
- de Almeida, U. Barres
- Bazer-Bachi, A. R.
- Becherini, Y.
- Behera, B.
Benbow, W. Bernloehr, K. Boisson, C. Bochow, A. - Zeige mehr (+4)…
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- Erscheinungsjahr:
- 2009
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- Text
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- Aims. Detection of a γ-ray source above 300 GeV is reported, confirming the unidentified source MGRO J1908+06, discovered by the Milagro collaboration at a median energy of 20 TeV. Methods. The source was observed during 27 h as part of the extension of the HESS Galactic plane survey to longitudes >30°. Results. HESS J108+063 is detected at a significance level of 10.9σ with an integral flux above 1 TeV of (3.76 ± 0.29 statPlusmn: 0.75sys) × 10-12 ph cm-2 s-1, and a spectral photon index Γ = 2.10 ± 0.07 stat ± 0.2sys. The positions and fluxes of HESS J1908+063 and MGRO J1908+06 are in good agreement. Possible counterparts at other wavelengths and the origin of the γ-ray emission are discussed. The nearby unidentified GeV source, GRO J1908+0556 (GeV) which also remains unidentified and the new Fermi pulsar 0FGL J1907.5+0617, may be connected to the TeV source. © ESO 2009.
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- info:eu-repo/semantics/openAccess
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- Forschungsinformationssystem der UHH
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