Probing the X-ray Emission from Dueling Magnetospheres

Details Probing the X-ray Emission from Dueling Magnetospheres Probing the X-ray Emission from Dueling Magnetospheres

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cxo..prop.1685c&link_type=abstract

Chandra Proposal ID #06400876

Physics

Chandra Proposal Id #06400876

Scientific paper

The double pulsar system J0737-3039 may provide answers to longstanding questions about the pulsar emission mechanism and the physics of relativistic winds. X-ray emission detected with Chandra could be produced by pulsed magnetospheric emission or at termination shocks located at the wind-wind boundary or the wind-ISM boundary. We propose high time resolution observations with HRC-S which will determine the X-ray modulation fraction at the pulsar rotational and orbital periods, thus distinguishing between the various possibilities and providing direct constraints on the magnetization parameter of the relativistic wind.

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