The role pulsar wind nebulae play in producing our locally observed cosmic ray spectrum remains murky, yet intriguing. Pulsar wind nebulae are born and evolve in conjunction with SNRs, which are favored sites of Galactic cosmic ray acceleration. As a result they frequently complicate interpretation of the gamma-ray emission seen from SNRs. However, pulsar wind nebulae may also contribute directly to the local cosmic ray spectrum, particularly the leptonic component. This paper reviews the current thinking on pulsar wind nebulae and their connection to cosmic ray production from an observational perspective. It also considers how both future technologies and new ways of analyzing existing data can help us to better address the relevant theor...
Observations of TeV gamma rays enable investigation of extreme, high-energy astrophysical environmen...
Recent advances in very-high-energy (VHE) gamma-ray astronomy have opened a new observational window...
Broadband emission has been detected from several pulsar wind nebulae (PWNe), however the physical p...
In the past few years, gamma-ray astronomy has entered a golden age thanks to two major breakthrough...
International audienceIn the past few years, gamma-ray astronomy has entered a golden age thanks to ...
International audienceIn the past few years, gamma-ray astronomy has entered a golden age thanks to ...
International audienceIn the past few years, gamma-ray astronomy has entered a golden age thanks to ...
International audienceIn the past few years, gamma-ray astronomy has entered a golden age thanks to ...
In the past few years, gamma-ray astronomy has entered a golden age thanks to two major breakthrough...
In the past few years, gamma-ray astronomy has entered a golden age thanks to two major breakthrough...
In the past few years, gamma-ray astronomy has entered a golden age thanks to two major breakthrough...
Pulsars have been known to exist for over forty years now, but the nature of their emission througho...
Observations of TeV gamma rays enable investigation of extreme, high-energy astrophysical environmen...
I will review the current status of our theoretical understanding of Pulsar Winds and associated neb...
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...
Recent advances in very-high-energy (VHE) gamma-ray astronomy have opened a new observational window...
Broadband emission has been detected from several pulsar wind nebulae (PWNe), however the physical p...
In the past few years, gamma-ray astronomy has entered a golden age thanks to two major breakthrough...
International audienceIn the past few years, gamma-ray astronomy has entered a golden age thanks to ...
International audienceIn the past few years, gamma-ray astronomy has entered a golden age thanks to ...
International audienceIn the past few years, gamma-ray astronomy has entered a golden age thanks to ...
International audienceIn the past few years, gamma-ray astronomy has entered a golden age thanks to ...
In the past few years, gamma-ray astronomy has entered a golden age thanks to two major breakthrough...
In the past few years, gamma-ray astronomy has entered a golden age thanks to two major breakthrough...
In the past few years, gamma-ray astronomy has entered a golden age thanks to two major breakthrough...
Pulsars have been known to exist for over forty years now, but the nature of their emission througho...
Observations of TeV gamma rays enable investigation of extreme, high-energy astrophysical environmen...
I will review the current status of our theoretical understanding of Pulsar Winds and associated neb...
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...
Recent advances in very-high-energy (VHE) gamma-ray astronomy have opened a new observational window...
Broadband emission has been detected from several pulsar wind nebulae (PWNe), however the physical p...