J
J.-P. Tavernet
Researcher at Université libre de Bruxelles
Publications - 1
Citations - 537
J.-P. Tavernet is an academic researcher from Université libre de Bruxelles. The author has contributed to research in topics: Cosmic ray & Supernova. The author has an hindex of 1, co-authored 1 publications receiving 522 citations. Previous affiliations of J.-P. Tavernet include Centre national de la recherche scientifique.
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High-energy particle acceleration in the shell of a supernova remnant.
Felix Aharonian,A. G. Akhperjanian,Klaus-Michael Aye,A. R. Bazer-Bachi,M. Beilicke,Wystan Benbow,David Berge,P. Berghaus,P. Berghaus,Konrad Bernlöhr,Konrad Bernlöhr,O. Bolz,Catherine Boisson,C. Borgmeier,F. Breitling,A. M. Brown,J. Bussons Gordo,P. M. Chadwick,V. R. Chitnis,V. R. Chitnis,L-M. Chounet,R. Cornils,Luigi Costamante,B. Degrange,A. Djannati-Ataï,L. O'c. Drury,Tulun Ergin,P. Espigat,F. Feinstein,P. Fleury,G. Fontaine,Stefan Funk,Y. A. Gallant,B. Giebels,Stefan Gillessen,P. Goret,Julien Guy,Julien Guy,C. Hadjichristidis,M. Hauser,G. Heinzelmann,Gilles Henri,German Hermann,Jim Hinton,Werner Hofmann,M. Holleran,Dieter Horns,O. C. de Jager,I. Jung,I. Jung,B. Khélifi,Nu. Komin,A. Konopelko,A. Konopelko,I. J. Latham,R. Le Gallou,M. Lemoine,A. Lemière,N. Leroy,Thomas Lohse,A. Marcowith,Conor Masterson,T. J. L. McComb,M. de Naurois,M. de Naurois,S. J. Nolan,A. Noutsos,K. J. Orford,J. L. Osborne,M. Ouchrif,M. Ouchrif,M. Panter,Guy Pelletier,S. Pita,Martin Pohl,Martin Pohl,G. Pühlhofer,Michael Punch,B. C. Raubenheimer,M. Raue,J. Raux,J. Raux,S. M. Rayner,I. Redondo,I. Redondo,A. Reimer,Olaf Reimer,J. Ripken,M. Rivoal,M. Rivoal,L. Rob,L. Rolland,L. Rolland,Gavin Rowell,V. Sahakian,L. Saugé,S. Schlenker,Reinhard Schlickeiser,C. Schuster,U. Schwanke,M. Siewert,Helene Sol,R. Steenkamp,C. Stegmann,J.-P. Tavernet,J.-P. Tavernet,C. G. Théoret,M. Tluczykont,D. J. van der Walt,G. Vasileiadis,P. Vincent,P. Vincent,B. Visser,Heinrich J. Völk,Stefan Wagner +114 more
TL;DR: A TeV γ-ray image of the SNR shows the spatially resolved remnant has a shell morphology similar to that seen in X-rays, which demonstrates that very-high-energy particles are accelerated there, consistent with current ideas of particle acceleration in young SNR shocks.