Deep XMM-Newton Observation of the Relativistic Double Pulsar PSR J0737-3039

Details Deep XMM-Newton Observation of the Relativistic Double Pulsar PSR J0737-3039 Deep XMM-Newton Observation of the Relativistic Double Pulsar PSR J0737-3039

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..191p&link_type=abstract

XMM-Newton Proposal ID #04051002

Other

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Psr J0737-3039, Psr J0737-3039, Xmm-Newton Proposal 04051002

Scientific paper

The binary radio pulsar J0737-3039 is a truly unique system offering the enormous diagnostics of two radio pulsars in a short orbital period system. The properties of these two neutron stars are being constrained with unprecedented precision. In particular, this system is a unique laboratory for the study of the pulsar magnetospheres and the interaction between the pulsars' relativistic winds. High-energy observations are necessary to give a complete picture of the processes. The low X-ray luminosity requires a very long exposure time, but the added value of the detailed modeling of these pulsars through observation at other wavelengths, makes this a worth investment. No other X-ray observatory of the current generation will be able to yield better information.

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