XMM-Newton Proposal 02019205

Details XMM-Newton Proposal 02019205 XMM-Newton Proposal 02019205

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..105c&link_type=abstract

XMM-Newton Proposal ID #02019205

Physics

Psr B1259-63, Psr B1259-63, Psr B1259-63, Psr B1259-63, Psr B1259-63, Xmm-Newton Proposal 02019205

Scientific paper

PSR B1259-63 is a unique binary system with a radio pulsar from which unpulsed X-ray and radio emission was observed. The pulsar is in a highly eccentric 3.4 year orbit with a Be star. The collision of the pulsar wind with the wind of Be star plays a crucial role in the generation of the observed emission. The goal of this proposal is to investigate the changes of the system emission as the pulsar approaches to the Be star disk, and with the help of the received data to reconstruct the physical processes governing the system.

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