Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Galaxy Astrophysics
Scientist
Sterrenkundig Instituut, Utrecht
Sterrenkundig Instituut Utrecht, Netherlands
CEA-Saclay
Montpellier
external author
Astronomical Institute, Utrecht University, 3508 TA Utrecht, Netherlands
Sterrenkundig Instituut Utrecht, Postbus 80000 Utrecht 3508 TA, The Netherlands
Laboratoire de Physique Théorique et Astroparticules, IN2P3 / CNRS, Université Montpellier II, France
Astronomical Institute, Utrecht University, PO Box 80000, 3508 TA Utrecht, The Netherlands; Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy; Service d'Astrophysique, CEA Saclay, 91191 Gif-sur-Yvette Cedex, France
Astronomical Institute, Utrecht University, Postbus 80 000, 3508 TA Utrecht, Netherlands
Lawrence Livermore National Lab., CA.
Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS / IN2P3, CC 70, Place Eugène Bataillon, 34095 Montpellier Cedex 5, France
LPTA, Universite Montpellier II, CNRS / IN2P3, Montpellier, France
Labo. de Physique Theorique et Astroparticules, Universite MontpellierII
Astronomical Institute, Utrecht University
Astronomical Institute, Utrecht University, P.O. Box 80 000, 3508 TA Utrecht, Netherlands
LPTA, Montpellier, France
UC Berkeley
CEA Saclay
Astronomical Institute Utrecht
CEA-Saclay, France
Laboratoire de Physique Théorique et Astroparticules, UMR 5027, CNRS / IN2P3, Université Montpellier II, 34095 Montpellier Cedex 5, France of Calilfornia, Berkeley, CA, US
Lawrence Livermore National Laboratory, Livermore, CA
Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland
LPTA, University Montpellier II, CNRS, France
A multiwavelength view of the flaring state of PKS 2155-304 in 2006
A new SNR with TeV shell-type morphology: HESS J1731-347
A Shocked Pulsar Wind Model of the Crab Nebula's Wisps
A wind model for high energy pulses
All-particle primary energy spectrum in the 3-200 PeV energy range
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