Other
Scientific paper
Sep 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.2046r&link_type=abstract
Chandra Proposal ID #07911006
Other
Chandra Proposal Id #07911006
Scientific paper
Recent X-ray and radio studies of unidentified high-energy gamma-ray source error boxes (detected by EGRET) have yielded numerous likely counterparts. These have been young pulsars coincident with steady EGRET sources, rapidly moving pulsar wind nebulae coincident with variable EGRET sources, and radio emitting Be X-ray binary "microquasars". We propose brief observations of 6 hard X-ray sources discovered in an ASCA survey of Galactic GeV source error boxes to determine if any are members of the above source classes or can be identified with other potential gamma-ray emitters.
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