Computer Science
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..616g&link_type=abstract
Chandra Proposal ID #02500775
Computer Science
Chandra Proposal Id #02500775
Scientific paper
We propose a deep ACIS imaging observation of the plerionic core of SNR CTB 80, containing PSR B1951+32. Our goals are: 1) to resolve the pulsar from a probable synchrotron nebula component associated with the radio `hot spot' and to determine their respective spectra, a task which is only possible with Chandra; 2) to detect or place upper limits on thermal emission from the bow shock surrounding the plerionic nebula; 3) to determine the temperature of the protruding `ears' of the core, thought to be the cocoons surrounding twin jets from the pulsar, and possibly detect these jets directly in X-rays. This measurement of the velocity of the shocks driven by the jets in a medium of known density could yield a solid determination of the bulk flow energy in pulsar jets.
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