Using Chandra to investigate the X-ray properties of the enigmatic, bipolar TeV source HESS J1841-053

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Chandra Proposal Id #08400470

Scientific paper

From a population of Galactic TeV gamma-ray sources newly detected with the H.E.S.S. telescope system, HESS J1841-053 is the only object which shows an extended, bipolar TeV morphology, together with an X-ray binary at the core of the source. We propose to use Chandra observations on the lobes of HESS J1841-053 to identify the nature of the TeV source and to verify its association with the central object. If the suggested identification holds, HESS J1841-053 would represent a new type of X-ray/TeV source.

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