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D. Sanwal, G. G. Pavlov, G. P. Garmire (Penn State University)
Thanks to the superb spatial resolution of Chandra, recent observations of several young pulsars (e.g., J1509--5850, J1809--1917, Geminga) have shown intriguing short (3''--10'') ``tails'' behind them. We will present the results of Chandra observations of these objects and discuss possible interpretations and the origin of the tails, including magnetospehric jets, confined wakes, and bow-shock surfaces.
This work was supported by SAO grant GO3-4075X, NASA grant NAG5-10865, and NASA contract NAS8-38252.
The author(s) of this abstract have provided an email address for comments about the abstract: divas@astro.psu.edu
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Bulletin of the American Astronomical Society, 37 #2
© 2005. The American Astronomical Soceity.