Speaker
Mr
Maxime REGEARD
(APC - CNRS)
Description
The recent discovery of multi-TeV pulsed emission from Vela and PSR J1509-5850 represents a major breakthrough in pulsar physics. We present the latest findings from very high-energy (VHE) observations using the H.E.S.S. telescopes and discuss key similarities and differences in the emission properties of these two pulsars in the GeV and multi-TeV ranges, in relation to their main characteristics. We then examine the implications for theoretical models describing high-energy pulsar emission. These results not only refine existing models but also pave the way for future TeV observations and studies of pulsars.
| Collaboration(s) | H.E.S.S. |
|---|
Authors
Arache Djannati-Ataï
(APC- CNRS)
Mr
Maxime REGEARD
(APC - CNRS)
