Resolving the Crab pulsar wind nebula at teraelectronvolt energies
- Abdalla, H.
- Aharonian, F.
- Ait Benkhali, F.
- Angüner, E.O.
- Arakawa, M.
- Arcaro, C.
- Armand, C.
- 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-Ataï, 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.
- Gaté, F.
- 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.
- Khangulyan, D.
- Khélifi, B.
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- Kluźniak, W.
- Komin, Nu.
- Kosack, K.
- Kraus, M.
- Lamanna, G.
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- Venter, C.
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- 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.
- Ziegler, A.
- Zorn, J.
- Żywucka, N.
DOIAbstract
International audienceThe Crab nebula is one of the most-studied cosmic particle accelerators, shining brightly across the entire electromagnetic spectrum up to very-high-energy gamma rays1,2. It is known from observations in the radio to gamma-ray part of the spectrum that the nebula is powered by a pulsar, which converts most of its rotational energy losses into a highly relativistic outflow. This outflow powers a pulsar wind nebula, a region of up to ten light-years across, filled with relativistic electrons and positrons. These particles emit synchrotron photons in the ambient magnetic field and produce very-high-energy gamma rays by Compton up-scattering of ambient low-energy photons. Although the synchrotron morphology of the nebula i...
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