Sep 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..275m&link_type=abstract
Chandra Proposal ID #01500136
Physics
Chandra Proposal Id #01500136
Scientific paper
Use the high spatial resolution of AXAF/HRC to separate possible pulsars
from surrounding nebular emission. Accurately measure the pulse fraction
and shape of any detected pulsars.
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