'Pulsar wind nebulae' diaporamas de présentation

The Cosmic Ray Electron Excess

580 views • 43 slides

Pulsar Wind Nebulae at High Energies

Pulsar Wind Nebulae at High Energies. Stephen C.-Y. Ng HKU. Outline. What are pulsar wind nebulae? Physical properties and evolution Why study PWNe ? Common TeV sources, particle accelerators Multiwavelength observations of PWNe Broadband SED Surprise from Fermi : Crab flaring.

722 views • 42 slides

MA4: HIGH-ENERGY ASTROPHYSICS

415 views • 26 slides

MA4: HIGH-ENERGY ASTROPHYSICS

387 views • 26 slides

Relaxation of Pulsar Wind Nebula via Current-Driven Kink Instability

Relaxation of Pulsar Wind Nebula via Current-Driven Kink Instability. Yosuke Mizuno ( ?? ?? ) Institute of Astronomy National Tsing-Hua University Collaborators Y. Lyubarsky (Ben-Gurion Univ), K.-I. Nishikawa (NSSTC/UAH), P. E. Hardee (Univ. of Alabama, Tuscaloosa).

253 views • 25 slides

VERITAS Observations of Supernova Remnants and Pulsar Wind Nebulae in the Fermi Era

336 views • 17 slides

Spectral Softening In Magnetic Bubbles

Spectral Softening In Magnetic Bubbles. Pulsar. +. G. +. +. +. +. R. Pulsar Wind Nebulae. b. }. Pulsar. logarithmic radial scale. Crab Nebula. Wind. Shock. MHD. Blast Wave. Particle Flow. H a or ejecta shell. Lu et al. 2002. G5.4-0.1. PWN G18.0-0.7. PWN G18.0-0.7.

285 views • 17 slides

VERITAS Observations of Supernova Remnants and Pulsar Wind Nebulae in the Fermi Era

176 views • 17 slides