Add to ORKGPulsar wind nebulae (PWNe) are extended structures of shocked relativistic particules powered by a pulsar at very high energy. Interaction between these particules and the surrounding medium produces very high energy photons emission. Observation by imaging Cherenkov telescopes system in an energy scale from about 100 GeV to 100 TeV, shows various morphologies, depending of many parameters : age, ambiant medium distribution, magnetic fields. H.E.S.S. experiment enabled to find out many sources, like Vela X or HESS J1825-137, usefull for morphology analysis. In this talk, I will present last results got with H.E.S.S. and implication with evolution model of PWNe
International audienceThe most numerous TeV sources in the Milky Way are pulsar wind nebulae (PWNe);...
We present the discovery of two very-high-energy gamma-ray sources in an ongoing systematic search f...
The H.E.S.S. detector is an array of atmospheric-Cherenkov telescopes dedicated to the observation o...
Pulsar wind nebulae (PWNe) are extended structures of shocked relativistic particules powered by a p...
Recent advances in very-high-energy (VHE) gamma-ray astronomy have opened a new observational window...
Pulsars energise particles into lighthouse pencil beams and create extended relativistic outflows, p...
The observation of Very-High-Energy (vhe, >100 GeV) gamma rays is key in studying the non-thermal so...
Observations of TeV gamma rays enable investigation of extreme, high-energy astrophysical environmen...
International audienceThe most numerous TeV sources in the Milky Way are pulsar wind nebulae (PWNe);...
We present the discovery of two very-high-energy gamma-ray sources in an ongoing systematic search f...
The H.E.S.S. detector is an array of atmospheric-Cherenkov telescopes dedicated to the observation o...
Pulsar wind nebulae (PWNe) are extended structures of shocked relativistic particules powered by a p...
Recent advances in very-high-energy (VHE) gamma-ray astronomy have opened a new observational window...
Pulsars energise particles into lighthouse pencil beams and create extended relativistic outflows, p...
The observation of Very-High-Energy (vhe, >100 GeV) gamma rays is key in studying the non-thermal so...
Observations of TeV gamma rays enable investigation of extreme, high-energy astrophysical environmen...
International audienceThe most numerous TeV sources in the Milky Way are pulsar wind nebulae (PWNe);...
We present the discovery of two very-high-energy gamma-ray sources in an ongoing systematic search f...
The H.E.S.S. detector is an array of atmospheric-Cherenkov telescopes dedicated to the observation o...