Details

Autor(en) / Beteiligte

• Aharonian, F.
• Benkhali, F. A.
• Anguner, E.
• Balenderan, S.
• Barnacka, A.
• Birsin, E.
• Bottcher, M.
• Bolmont, J.
• Bordas, P.
• Brucker, J.
• Carrigan, S.
• Casanova, S.
• Cerruti, M.
• Chalme-Calvet, R.
• Conrad, J.
• Couturier, C.
• Dalton, M.
• Davids, I. D.
• Deil, C.
• deWilt, P.
• Dickinson, H. J.
• Dutson, K.
• Dyks, J.
• Egberts, K.
• Espigat, P.
• Farnier, C.
• Fegan, S.
• Fernandes, M. V.
• Fernandez, D.
• Forster, A.
• Fussling, M.
• Gajdus, M.
• Garrigoux, T.
• Grondin, M.- H.
• Hermann, G.
• Hofmann, W.
• Hofverberg, P.
• Holler, M.
• Jahn, C.
• Jamrozy, M.
• Janiak, M.
• Jankowsky, F.
• Kastendieck, M. A.
• Katz, U.
• Kaufmann, S.
• Kieffer, M.
• Kneiske, T.
• Kolitzus, D.
• Krayzel, F.
• Kruger, P. P.
• Lamanna, G.
• Lefaucheur, J.
• Lemiere, A.
• Lemoine-Goumard, M.
• Lohse, T.
• Maxted, N.
• Mayer, M.
• Menzler, U.
• Meyer, M.
• Moulin, E.
• Naumann, C. L.
• de Naurois, M.
• Niemiec, J.
• Nolan, S. J.
• Wilhelmi, E. d. O.
• Ostrowski, M.
• Oya, I.
• Panter, M.
• Parsons, R. D.
• Arribas, M. P.
• Perez, J.
• Pita, S.
• Puhlhofer, G.
• Quirrenbach, A.
• Raue, M.
• Reimer, A.
• Renaud, M.
• Rudak, B.
• Sahakian, V.
• Schlickeiser, R.
• Schulz, A.
• Schwanke, U.
• Schwemmer, S.
• Steenkamp, R.
• Stegmann, C.
• Szostek, A.
• Tavernier, T.
• Tluczykont, M.
• van Eldik, C.
• van Soelen, B.
• Vasileiadis, G.
• Viana, A.
• Vink, J.
• Wagner, S. J.
• Wagner, P.
• Weitzel, Q.
• Wornlein, A.
• Wouters, D.
• Zech, A.
• Zechlin, H.- S.

Titel

HESS J1640-465 - an exceptionally luminous TeV  -ray supernova remnant

Ist Teil von

• Monthly notices of the Royal Astronomical Society, 2014-04, Vol.439 (3), p.2828-2836

Ort / Verlag

London: Oxford University Press

Erscheinungsjahr

2014

Quelle

Alma/SFX Local Collection

Beschreibungen/Notizen

• The results of follow-up observations of the TeV ...-ray source HESS J1640-465 from 2004 to 2011 with the High Energy Stereoscopic System (HESS) are reported in this work. The spectrum is well described by an exponential cut-off power law with photon index ... = 2.11 ± 0.09... ± 0.10..., and a cut-off energy of E...=6.0... TeV. The TeV emission is significantly extended and overlaps with the northwestern part of the shell of the SNR G338.3-0.0. The new HESS results, a re-analysis of archival XMM-Newton data and multiwavelength observations suggest that a significant part of the ...-ray emission from HESS J1640-465 originates in the supernova remnant shell. In a hadronic scenario, as suggested by the smooth connection of the GeV and TeV spectra, the product of total proton energy and mean target density could be as high as WpnH ~ 4 x 10...(d/10kpc)... erg cm... (ProQuest: ... denotes formulae/symbols omitted.)