a Small Chandra Survey of Hard X-Ray Sources in Gamma-Ray Error Boxes

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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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