Do Some Critters Play Frisbee? Observations of Various Pulsars and Their Nebulae

Details Do Some Critters Play Frisbee? Observations of Various Pulsars and Their Nebulae Do Some Critters Play Frisbee? Observations of Various Pulsars and Their Nebulae

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011head...12.2607r&link_type=abstract

American Astronomical Society, HEAD meeting #12, #26.07

Astronomy and Astrophysics

Astronomy

Scientific paper

We present X-ray imaging observations of several pulsars and their wind nebulae, comparing them to radio images where appropriate. While most pulsar wind nebulae have either a torus+jet morphology or a bow shock/tail morphology, in some cases it appears there is a hybrid morphology where on large scales there is a bow shape from their motion, and on smaller scales a torus+jet morphology which is tilted and offset with respect to the symmetry axis of the apparent bow shock. We present a simple model of the effects of an equatorially enhanced wind on a ram-pressure confined nebula. We discuss implications of this picture for birth sites and potentially related TeV sources.

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