| Issue |
EPJ Web Conf.
Volume 136, 2017
RICAP16, 6th Roma International Conference on Astroparticle Physics
|
|
|---|---|---|
| Article Number | 03003 | |
| Number of page(s) | 4 | |
| Section | Gamma Rays | |
| DOI | https://doi.org/10.1051/epjconf/201713603003 | |
| Published online | 23 March 2017 | |
https://doi.org/10.1051/epjconf/201713603003
The Crab pulsar at VHE
Max-Planck-Institut fur Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany
a e-mail: Roberta.Zanin@mpi-hd.mpg.de
Published online: 23 March 2017
The last six years have witnessed major revisions of our knowledge about the Crab Pulsar. The consensus scenario for the origin of the high-energy pulsed emission has been challenged with the discovery of a very-high-energy power law tail extending up to ~400 GeV, above the expected spectral cut off at a few GeV. Now, new measurements obtained by the MAGIC collaboration extend the energy spectrum of the Crab Pulsar even further, on the TeV regime. Above ~400 GeV the pulsed emission comes mainly from the interpulse, which becomes more prominent with energy due to a harder spectral index. These findings require γ -ray production via inverse Compton scattering close to or beyond the light cylinder radius by an underlying particle population with Lorentz factors greater than 5 × 106. We will present those new results and discuss the implications in our current knowledge concerning pulsar environments.
© The Authors, published by EDP Sciences, 2017
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