Mapping the Magnetic Field Structure and Morphology of Pulsar Bow Shocks and Wind Nebulae

Details Mapping the Magnetic Field Structure and Morphology of Pulsar Bow Shocks and Wind Nebulae Mapping the Magnetic Field Structure and Morphology of Pulsar Bow Shocks and Wind Nebulae

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atnf.prop.1867n&link_type=abstract

ATNF proposal C1979, Semester: October, 2008

Other

Galactic, Atca

Scientific paper

We propose ATCA observations of five pulsar wind nebula (PWN) candidates
in order to determine their magnetic field structure and map the nebular
morphology. By comparing these observations to simulations and other PWN
examples, we will obtain a better understanding of relativistic shocks
and the electrodynamics of pulsar winds.

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