Particle Transport within the Pulsar Wind Nebula HESS J1825-137
- Abdalla, H.
- Aharonian, F.
- Ait Benkhali, F.
- Angüner, E.O.
- Arakawa, M.
- Arcaro, C.
- Armand, C.
- Arrieta, M.
- Backes, M.
- Barnard, M.
- Becherini, Y.
- Becker Tjus, J.
- Berge, D.
- Bernlöhr, K.
- Blackwell, R.
- Böttcher, M.
- Boisson, C.
- Bolmont, J.
- Bonnefoy, S.
- Bordas, P.
- Bregeon, J.
- Brun, F.
- Brun, P.
- Bryan, M.
- Büchele, M.
- Bulik, T.
- Bylund, T.
- Capasso, M.
- Caroff, S.
- Carosi, A.
- Casanova, S.
- Cerruti, M.
- Chakraborty, N.
- Chand, T.
- Chandra, S.
- Chaves, R.C.G.
- Chen, A.
- Colafrancesco, S.
- Condon, B.
- Davids, I.D.
- Deil, C.
- Devin, J.
- Dewilt, P.
- Dirson, L.
- Djannati-Atai, A.
- Dmytriiev, A.
- Donath, A.
- Doroshenko, V.
- Drury, L.O'C.
- Dyks, J.
- Egberts, K.
- Emery, G.
- Ernenwein, J.-P.
- Eschbach, S.
- Fegan, S.
- Fiasson, A.
- Fontaine, G.
- Funk, S.
- Füssling, M.
- Gabici, S.
- Gallant, Y.A.
- Giavitto, G.
- Glawion, D.
- Glicenstein, J.F.
- Gottschall, D.
- Grondin, M.-H.
- Hahn, J.
- Haupt, M.
- Heinzelmann, G.
- Henri, G.
- Hermann, G.
- Hinton, J.A.
- Hofmann, W.
- Hoischen, C.
- Holch, T.L.
- Holler, M.
- Horns, D.
- Huber, D.
- Iwasaki, H.
- Jacholkowska, A.
- Jamrozy, M.
- Jankowsky, D.
- Jankowsky, F.
- Jouvin, L.
- Jung-Richardt, I.
- Kastendieck, M.A.
- Katarzyński, K.
- Katsuragawa, M.
- Katz, U.
- Kerszberg, D.
- Khangulyan, D.
- Khélifi, B.
- King, J.
- Klepser, S.
- Kluźniak, W.
- Komin, Nu.
- Kosack, K.
- Kraus, M.
- Lamanna, G.
- Lau, J.
- Lefaucheur, J.
- Lemière, A.
- Lemoine-Goumard, M.
- Lenain, J.-P.
- Leser, E.
- Lohse, T.
- López-Coto, R.
- Lypova, I.
- Malyshev, D.
- Marandon, V.
- Marcowith, Alexandre
- Mariaud, C.
- Martí-Devesa, G.
- Marx, R.
- Maurin, G.
- Meintjes, P.J.
- Mitchell, A.M.W.
- Moderski, R.
- Mohamed, M.
- Mohrmann, L.
- Moore, C.
- Moulin, E.
- Murach, T.
- Nakashima, S.
- de Naurois, M.
- Ndiyavala, H.
- Niederwanger, F.
- Niemiec, J.
- Oakes, L.
- O'Brien, P.
- Odaka, H.
- Ohm, S.
- Ostrowski, M.
- Oya, I.
- Panter, M.
- Parsons, R.D.
- Perennes, C.
- Petrucci, P.-O.
- Peyaud, B.
- Piel, Q.
- Pita, S.
- Poireau, V.
- Priyana Noel, A.
- Prokhorov, D.A.
- Prokoph, H.
- Pühlhofer, G.
- Punch, M.
- Quirrenbach, A.
- Raab, S.
- Rauth, R.
- Reimer, A.
- Reimer, O.
- Renaud, Matthieu
- Rieger, F.
- Rinchiuso, L.
- Romoli, C.
- Rowell, G.
- Rudak, B.
- Ruiz-Velasco, E.
- Sahakian, V.
- Saito, S.
- Sanchez, D.A.
- Santangelo, A.
- Sasaki, M.
- Schlickeiser, R.
- Schüssler, F.
- Schulz, A.
- Schutte, H.
- Schwanke, U.
- Schwemmer, S.
- Seglar-Arroyo, M.
- Senniappan, M.
- Seyffert, A.S.
- Shafi, N.
- Shilon, I.
- Shiningayamwe, K.
- Simoni, R.
- Sinha, A.
- Sol, H.
- Specovius, A.
- Spir-Jacob, M.
- Stawarz, L.
- Steenkamp, R.
- Stegmann, C.
- Steppa, C.
- Takahashi, T.
- Tavernet, J.-P.
- Tavernier, T.
- Taylor, A.M.
- Terrier, R.
- Tibaldo, L.
- Tiziani, D.
- Tluczykont, M.
- Trichard, C.
- Tsirou, M.
- Tsuji, N.
- Tuffs, R.
- Uchiyama, Y.
- van Der Walt, D.J.
- van Eldik, C.
- van Rensburg, C.
- van Soelen, B.
- Vasileiadis, George
- Veh, J.
- Venter, C.
- Vincent, P.
- Vink, J.
- Voisin, F.
- Völk, H.J.
- Vuillaume, T.
- Wadiasingh, Z.
- Wagner, S.J.
- Wagner, R.M.
- White, R.
- Wierzcholska, A.
- Yang, R.
- Yoneda, H.
- Zaborov, D.
- Zacharias, M.
- Zanin, R.
- Zdziarski, A.A.
- Zech, A.
- Zefi, F.
- Ziegler, A.
- Zorn, J.
- Żywucka, N.
DOIAbstract
International audienceContext. We present a detailed view of the pulsar wind nebula (PWN) HESS J1825–137. We aim to constrain the mechanisms dominating the particle transport within the nebula, accounting for its anomalously large size and spectral characteristics.Aims. The nebula was studied using a deep exposure from over 12 years of H.E.S.S. I operation, together with data from H.E.S.S. II that improve the low-energy sensitivity. Enhanced energy-dependent morphological and spatially resolved spectral analyses probe the very high energy (VHE, E > 0.1 TeV) γ-ray properties of the nebula.Methods. The nebula emission is revealed to extend out to 1.5° from the pulsar, ~1.5 times farther than previously seen, making HESS J1825–137, with an int...
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