XMM-Newton Proposal 03017401

Details XMM-Newton Proposal 03017401 XMM-Newton Proposal 03017401

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...58g&link_type=abstract

XMM-Newton Proposal ID #03017401

Computer Science

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, Psr B1338-62, Xmm-Newton Proposal 03017401

Scientific paper

PSR B1338-62 is a young radio pulsar coincident with the unusual supernova remnant (SNR) G308.8-0.1. Motivated by Chandra images of a similar young pulsar/SNR system in which the pulsar interacts with its SNR through a relativistic jet, we propose that PSR B1338-62 is associated with SNR G308.8-0.1, and powers a collimated outflow which is re-energising the SNR. We were awarded AO2 XMM observations to test this possibility, but the data were severely compromised by high radiation levels. We here repropose this experiment.

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