Physics
Scientific paper
Sep 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2383g&link_type=abstract
Chandra Proposal ID #09500030
Physics
Chandra Proposal Id #09500030
Scientific paper
We propose to observe a number of energetic, young, radio pulsars that has not yet been studied in X-rays. The pulsars and their wind nebulae are especially interesting since they are expected to be the GeV and TeV sources detectable in the near future with the Glast and HESS observatories. In the short, 10 ks, exposures we expect to detect emission from the pulsars and PWNe in all cases. Obtained images and spectra will allow us to select the brightest, most interesting objects for more detailed follow-up studies.
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