Probing the Magnetic Field in the GW170817 Outflow Using H.E.S.S. Observations
- ABDALLA, H.
- ADAM, R.
- AHARONIAN, F.
- BENKHALI, F. Ait
- ANGÜNER, E.O.
- ARAKAWA, M.
- ARCARO, C.
- ARMAND, C.
- ARMSTRONG, T.
- ASHKAR, H.
- BACKES, M.
- BAGHMANYAN, V.
- BARBOSA-MARTINS, V.
- BARNACKA, A.
- BARNARD, M.
- BECHERINI, Y.
- BERGE, D.
- BERNLÖHR, K.
- BLACKWELL, R.
- BÖTTCHER, M.
- BOISSON, C.
- BOLMONT, J.
- BONNEFOY, S.
- BREGEON, J.
- BREUHAUS, M.
- BRUN, F.
- BRUN, P.
- BRYAN, M.
- BÜCHELE, M.
- BULIK, T.
- BYLUND, T.
- CAROFF, S.
- CAROSI, A.
- CASANOVA, S.
- CERRUTI, M.
- CHAND, T.
- CHANDRA, S.
- CHEN, A.
- COTTER, G.
- CURYŁO, M.
- DAVIDS, I.D.
- DAVIES, J.
- DEIL, C.
- DEVIN, J.
- DEWILT, P.
- DIRSON, L.
- DJANNATI-ATAÏ, A.
- DMYTRIIEV, A.
- DONATH, A.
- DOROSHENKO, V.
- DYKS, J.
- EGBERTS, K.
- EICHHORN, F.
- EMERY, G.
- ERNENWEIN, J.-P.
- ESCHBACH, S.
- FEIJEN, K.
- FEGAN, S.
- FIASSON, A.
- FONTAINE, G.
- FUNK, S.
- FÜSSLING, M.
- GABICI, S.
- GALLANT, Y.A.
- GIAVITTO, G.
- GIUNTI, L.
- GLAWION, D.
- GLICENSTEIN, J.F.
- GOTTSCHALL, D.
- GRONDIN, M.-H.
- HAHN, J.
- HAUPT, M.
- HEINZELMANN, G.
- HERMANN, G.
- HINTON, J.A.
- HOFMANN, W.
- HOISCHEN, C.
- HOLCH, T.L.
- HOLLER, M.
- HÖRBE, M.
- HORNS, D.
- HUBER, D.
- IWASAKI, H.
- JAMROZY, M.
- JANKOWSKY, D.
- JANKOWSKY, F.
- JARDIN-BLICQ, A.
- JOSHI, V.
- JUNG-RICHARDT, I.
- KASTENDIECK, M.A.
- KATARZYŃSKI, K.
- KATSURAGAWA, M.
- KATZ, U.
- KHANGULYAN, D.
- KHÉLIFI, B.
- KLEPSER, S.
- KLUŹNIAK, W.
- KOMIN, Nu.
- KONNO, R.
- KOSACK, K.
- KOSTUNIN, D.
- KRETER, M.
- LAMANNA, G.
- LEMIÈRE, A.
- LEMOINE-GOUMARD, M.
- LENAIN, J.-P.
- LESER, E.
- LEVY, C.
- LOHSE, T.
- LYPOVA, I.
- MACKEY, J.
- MAJUMDAR, J.
- MALYSHEV, D.
- MARANDON, V.
- MARCHEGIANI, P.
- MARCOWITH, A.
- MARES, A.
- MARTÍ-DEVESA, G.
- MARX, R.
- MAURIN, G.
- MEINTJES, P.J.
- MODERSKI, R.
- MOHAMED, M.
- MOHRMANN, L.
- MOORE, C.
- MORRIS, P.
- MOULIN, E.
- MULLER, J.
- MURACH, T.
- NAKASHIMA, S.
- NAKASHIMA, K.
- DE NAUROIS, M.
- NDIYAVALA, H.
- NIEDERWANGER, F.
- NIEMIEC, J.
- OAKES, L.
- O'BRIEN, P.
- ODAKA, H.
- OHM, S.
- DE ONA WILHELMI, E.
- OSTROWSKI, M.
- PANTER, M.
- PARSONS, R.D.
- PEYAUD, B.
- PIEL, Q.
- PITA, S.
- POIREAU, V.
- NOEL, A. Priyana
- PROKHOROV, D.A.
- PROKOPH, H.
- PÜHLHOFER, G.
- PUNCH, M.
- QUIRRENBACH, A.
- RAAB, S.
- RAUTH, R.
- REIMER, A.
- REIMER, O.
- REMY, Q.
- RENAUD, M.
- RIEGER, F.
- RINCHIUSO, L.
- ROMOLI, C.
- ROWELL, G.
- RUDAK, B.
- RUIZ-VELASCO, E.
- SAHAKIAN, V.
- SAILER, S.
- SAITO, S.
- SANCHEZ, D.A.
- SANTANGELO, A.
- SASAKI, M.
- SCALICI, M.
- SCHLICKEISER, R.
- SCHÜSSLER, F.
- SCHULZ, A.
- SCHUTTE, H.M.
- SCHWANKE, U.
- SCHWEMMER, S.
- SEGLAR-ARROYO, M.
- SENNIAPPAN, M.
- SEYFFERT, A.S.
- SHAFI, N.
- SHININGAYAMWE, K.
- SIMONI, R.
- SINHA, A.
- SOL, H.
- SPECOVIUS, A.
- SPENCER, S.
- SPIR-JACOB, M.
- STAWARZ, Ł.
- STEENKAMP, R.
- STEGMANN, C.
- STEPPA, C.
- TAKAHASHI, T.
- TAVERNIER, T.
- TAYLOR, A.M.
- TERRIER, R.
- TIZIANI, D.
- TLUCZYKONT, M.
- TOMANKOVA, L.
- 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, G.
- VEH, J.
- VENTER, C.
- VINCENT, P.
- VINK, J.
- VÖLK, H.J.
- VUILLAUME, T.
- WADIASINGH, Z.
- WAGNER, S.J.
- WATSON, J.
- WERNER, Félix
- WHITE, R.
- WIERZCHOLSKA, A.
- YANG, R.
- YONEDA, H.
- ZACHARIAS, M.
- ZANIN, R.
- ZDZIARSKI, A.A.
- ZECH, A.
- ZORN, J.
- ŻYWUCKA, N.
- RODRIGUES, X.
DOIAbstract
The detection of the first electromagnetic counterpart to the binary neutron star (BNS) merger remnant GW170817 established the connection between short γ-ray bursts and BNS mergers. It also confirmed the forging of heavy elements in the ejecta (a so-called kilonova) via the r-process nucleosynthesis. The appearance of nonthermal radio and X-ray emission, as well as the brightening, which lasted more than 100 days, were somewhat unexpected. Current theoretical models attempt to explain this temporal behavior as either originating from a relativistic off-axis jet or a kilonova-like outflow. In either scenario, there is some ambiguity regarding how much energy is transported in the nonthermal electrons versus the magnetic field of the emissio...
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