Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21511701s&link_type=abstract
American Astronomical Society, AAS Meeting #215, #117.01; Bulletin of the American Astronomical Society, Vol. 42, p.605
Astronomy and Astrophysics
Astronomy
Scientific paper
The extended nebulae formed as pulsar winds expand into their surroundings provide information about the composition of the winds, the injection history from the host pulsar, and the material into which the nebulae are expanding. Observations from across the electromagnetic spectrum provide constraints on the evolution of the nebulae, the density and composition of the surrounding ejecta, the geometry of the central engines, and the long-term fate of the energetic particles produced in these systems. Such observations reveal the presence of jets and wind termination shocks, time-varying compact emission structures, shocked supernova ejecta, and newly formed dust. Here I provide a broad overview of the structure of pulsar wind nebulae, with specific examples from observations extending from the radio band to very high energy gamma-rays that demonstrate our ability to constrain the history and ultimate fate of the energy released in the spin-down of young pulsars.
No associations
LandOfFree
The Structure and Evolution of Pulsar Wind Nebulae does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Structure and Evolution of Pulsar Wind Nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Structure and Evolution of Pulsar Wind Nebulae will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-960861