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  A detailed spectral and morphological study of the gamma-ray supernova remnant RX J1713.7-3946 with HESS

Aharonian, F., Akhperjanian, A. G., Bazer-Bachi, A. R., Beilicke, M., Benbow, W., Berge, D., et al. (2006). A detailed spectral and morphological study of the gamma-ray supernova remnant RX J1713.7-3946 with HESS. Astronomy and Astrophysics, 449(1), 223-242. doi:10.1051/0004-6361:20054279.

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Aharonian, F.1, Author           
Akhperjanian, A. G.1, Author           
Bazer-Bachi, A. R.2, Author
Beilicke, M.1, Author           
Benbow, W.1, Author           
Berge, D.1, Author           
Borrel, V.2, Author
Bernlöhr, K.1, Author           
Bolz, O.1, Author           
Boisson, C:2, Author
Glicenstein, J.F.1, Author           
Breitling, F.2, Author
Brown, A. M.2, Author
Dickinson, H.J.2, Author
Chadwick, P. M.2, Author
Braun, I.1, Author           
Chounet, L.-M.2, Author
Cornils, R.1, Author           
Costamante, L.1, Author           
Degrange, B.2, Author
Djannati-Atai, A.1, Author           Drury, L.O'C.2, AuthorEmmanoulopoulos, D.2, AuthorEspigat, P.2, AuthorFeinstein, F.1, Author           Jacholkowska, A.2, AuthorFontaine, G.2, AuthorFunk, S.1, Author           Gallant, Y. A.1, Author           Giebels, B.2, AuthorGillessen, S.1, Author           Goret, P.2, AuthorDubus, G.1, Author           Hadjichristidis, C.2, AuthorHauser, M.2, AuthorHeinzelmann, G.2, AuthorHenri, G.2, AuthorHermann, G.1, Author           Hinton, J. A.1, Author           Hofmann, W.1, Author           Holleran, M.2, AuthorHorns, D.1, Author           de Jager, O. C.2, AuthorKhélifi, B.1, Author           Komin, N.2, AuthorKonopelko, A.3, Author           Latham, I. J.2, AuthorLe Gallou, R.2, AuthorLemoine-Goumard, M.2, AuthorLemière, A.2, AuthorLeroy, N.2, AuthorLohse, T.2, AuthorMarcowith, A.2, AuthorMasterson, C.1, Author           McComb, T. J. L.2, Authorde Naurois, M.1, Author           Nolan, S. J.2, AuthorNoutsos, A.2, AuthorOrford, K. J.1, Author           Osborne, J. L.1, Author           Ouchrif, M.2, AuthorPanter, M.1, Author           Pelletier, G.2, AuthorPita, S.2, AuthorFuchs, Y.2, AuthorPühlhofer, G.1, Author           Punch, M.2, AuthorRaubenheimer, B. C.2, AuthorRaue, M.1, Author           Raux, J.2, AuthorRayner, S. M.2, AuthorMartin, J.M.2, AuthorReimer, A.2, AuthorReimer, O.2, AuthorRipken, J.2, AuthorTerrier, R.2, AuthorRob, L.2, AuthorRolland, L.2, AuthorRowell, G.1, Author           Sahakian, V.2, AuthorSaugé, L.1, Author           Schlenker, S.2, AuthorSchlickeiser, R.2, AuthorSchuster, C.2, AuthorSchwanke, U.2, AuthorSiewert, M.2, AuthorSol, H.2, AuthorSteenkamp, R.2, AuthorStegmann, C.2, AuthorTavernet, J.-P-2, AuthorThéoret, C. G.2, AuthorTluczykont, M.2, AuthorVenter, C.2, AuthorVasileiadis, G.1, Author           Vincent, P.2, AuthorVölk, H. J.3, Author           Wagner, S. J.2, AuthorMartineau-Huynh, O.2, AuthorSpangler, D.2, Author more..
Affiliations:
1Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550              
2Yerevan Physics Institute, 2 Alikhanian Brothers Street, 375036 Yerevan, Armenia. Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK. Centre d'Etude Spatiale des Rayonnements, CNRS/UPS, 9 av. du Colonel Roche, BP 4346, F-31029 Toulouse Cedex 4, France. Institut für Experimentalphysik, Universität Hamburg, Luruper Chaussee 149, D-22761 Hamburg, Germany. APC, UMR 7164 du CNRS, 11 Place Marcelin Berthelot, F-75231 Paris Cedex 05, France. Institut für Physik, Humboldt-Universität zu Berlin, Newtonstr. 15, D-12489 Berlin, Germany. Laboratoire Univers et Théories (LUTH), UMR 8102 du CNRS, Observatoire de Paris, Section de Meudon, F-92195 Meudon Cedex, France. Laboratoire de Physique Théorique et Astroparticules, IN2P3/CNRS, Université Montpellier II, CC 70, Place Eugène Bataillon, F-34095 Montpellier Cedex 5, France. Laboratoire Leprince-Ringuet, IN2P3/CNRS, Ecole Polytechnique, F-91128 Palaiseau, France. Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland. Landessternwarte, Königstuhl, D-69117 Heidelberg, Germany. Laboratoire d'Astrophysique de Grenoble, INSU/CNRS, Université Joseph Fourier, BP 53, F-38041 Grenoble Cedex 9, France. DAPNIA/DSM/CEA, CE Saclay, F-91191 Gif-sur-Yvette, France. Unit for Space Physics, North-West University, Potchefstroom 2520, South Africa. Laboratoire de Physique Nucléaire et de Hautes Energies, IN2P3/CNRS, Universités Paris VI & VII, 4 Place Jussieu, F-75252 Paris Cedex 05, France. Institut für Theoretische Physik, Lehrstuhl IV: Weltraum und Astrophysik, Ruhr-Universität Bochum, D-44780 Bochum, Germany. Institute of Particle and Nuclear Physics (IPNP), Charles University, V Holesovickach 2, 180 00 Prague 8, Czech Republic. University of Namibia, Private Bag 13301, Windhoek, Namibia., ou_persistent22              
3Prof. Heinrich J. Völk, Emeriti, MPI for Nuclear Physics, Max Planck Society, ou_907548              

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Free keywords: acceleration of particles -- ISM: cosmic rays -- gamma rays: observations -- ISM: supernova remnants -- ISM: individual objects: RX J1713.7-3946 ( G347.3-0.5 ) H.E.S.S.
 Abstract: We present results from deep observations of the Galactic shell-type supernova remnant (SNR) RX J1713.7-3946 (also known as G347.3-0.5 ) conducted with the complete HESS array in 2004. Methods.Detailed morphological and spatially resolved spectral studies reveal the very-high-energy (VHE - Energies E > 100 GeV) gamma-ray aspects of this object with unprecedented precision. Since this is the first in-depth analysis of an extended VHE gamma-ray source, we present a thorough discussion of our methodology and investigations of possible sources of systematic errors. Results.Gamma rays are detected throughout the whole SNR. The emission is found to resemble a shell structure with increased fluxes from the western and northwestern parts. The differential gamma-ray spectrum of the whole SNR is measured over more than two orders of magnitude, from 190 GeV to 40 TeV, and is rather hard with indications for a deviation from a pure power law at high energies. Spectra have also been determined for spatially separated regions of RX J1713.7-3946 . The flux values vary by more than a factor of two, but no significant change in spectral shape is found. There is a striking correlation between the X-ray and the gamma-ray image. Radial profiles in both wavelength regimes reveal the same shape almost everywhere in the region of the SNR. Conclusions.The VHE gamma-ray emission of RX J1713.7-3946 is phenomenologically discussed for two scenarios, one where the gamma rays are produced by VHE electrons via Inverse Compton scattering and one where the gamma rays are due to neutral pion decay from proton-proton interactions. In conjunction with multi-wavelength considerations, the latter case is favoured. However, no decisive conclusions can yet be drawn regarding the parent particle population dominantly responsible for the gamma-ray emission from RX J1713.7-3946 .

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Language(s): eng - English
 Dates: 2006-04-01
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: eDoc: 276607
DOI: 10.1051/0004-6361:20054279
 Degree: -

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Title: Astronomy and Astrophysics
  Alternative Title : A&A
Source Genre: Journal
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Pages: - Volume / Issue: 449 (1) Sequence Number: - Start / End Page: 223 - 242 Identifier: -