The Unique Dynamical Vela Pulsar Wind Nebula

Details The Unique Dynamical Vela Pulsar Wind Nebula The Unique Dynamical Vela Pulsar Wind Nebula

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cxo..prop.2609p&link_type=abstract

Chandra proposal ID #10500817

Physics

Scientific paper

Chandra observations of the Vela pulsar-wind nebula (PWN) have revealed intriguing features in its structure and shown that the PWN brightness, shape, and spectrum change on a timescale as short as one week. Taking advantage of the known variability timescale, we propose a series of optimally sequenced observations to understand the PWN topology, dynamics, spectral structure, and interaction with the ambient matter.

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