Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/37439
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dc.contributor.author | Aharonian, F. | - |
dc.contributor.author | Akhperjanian, A. | - |
dc.contributor.author | Aye, K. | - |
dc.contributor.author | Bazer-Bachi, A. | - |
dc.contributor.author | Beilicke, M. | - |
dc.contributor.author | Benbow, W. | - |
dc.contributor.author | Berge, D. | - |
dc.contributor.author | Berghaus, P. | - |
dc.contributor.author | Bernlohr, K. | - |
dc.contributor.author | Boisson, C. | - |
dc.contributor.author | Bolz, O. | - |
dc.contributor.author | Borgmeier, C. | - |
dc.contributor.author | Braun, I. | - |
dc.contributor.author | Breitling, F. | - |
dc.contributor.author | Brown, A. | - |
dc.contributor.author | Bussons Gordo, J. | - |
dc.contributor.author | Chadwick, P. | - |
dc.contributor.author | Chounet, L. | - |
dc.contributor.author | Cornils, R. | - |
dc.contributor.author | Costamante, L. | - |
dc.contributor.author | et al. | - |
dc.date.issued | 2005 | - |
dc.identifier.citation | Astronomy and Astrophysics: a European journal, 2005; 432(2):L25-L29 | - |
dc.identifier.issn | 0004-6361 | - |
dc.identifier.issn | 1432-0746 | - |
dc.identifier.uri | http://hdl.handle.net/2440/37439 | - |
dc.description.abstract | Very high energy (>100 GeV) gamma-ray emission has been detected for the first time from the composite supernova remnant G 0.9+0.1 using the HESS instrument. The source is detected with a significance of ≈13σ, and a photon flux above 200 GeV of (5.7 ± 0.7 stat ± 1.2 sys) × 10 -12 cm -2 s -1, making it one of the weakest sources ever detected at TeV energies. The photon spectrum is compatible with a power law (dN/dE ∝ E Γ) with photon index Γ = 2.40 ± 0.11 stat ± 0.20 sys. The gamma-ray emission appears to originate in the plerionic core of the remnant, rather than the shell, and can be plausibly explained as inverse Compton scattering of relativistic electrons. © ESO 2005. | - |
dc.description.statementofresponsibility | F. Aharonian...G. Rowell...et al. | - |
dc.language.iso | en | - |
dc.publisher | E D P Sciences | - |
dc.rights | © The European Southern Observatory 2005 | - |
dc.source.uri | http://dx.doi.org/10.1051/0004-6361:200500022 | - |
dc.title | Very high energy gamma rays from the composite SNR G 0.9+0.1 | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1051/0004-6361:200500022 | - |
pubs.publication-status | Published | - |
dc.identifier.orcid | Rowell, G. [0000-0002-9516-1581] | - |
Appears in Collections: | Aurora harvest Chemistry and Physics publications |
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hdl_37439.pdf | Published version | 476.75 kB | Adobe PDF | View/Open |
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