Physics
Scientific paper
Oct 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..169c&link_type=abstract
XMM-Newton Proposal ID #05045502
Physics
White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Psr B1259-63, Psr B1259-63, Xmm-Newton Proposal 05045502
Scientific paper
PSR B1259-63 is a unique binary system with a radio pulsar from which unpulsed X-ray, Gamma-ray, and radio emission was observed. The pulsar is in a highly eccentric 3.4 year orbit around a Be star. Collision of the pulsar wind with the wind of Be star plays a crucial role in generation of the observed emission. The goal of this proposal is to investigate simultaneous radio-X-ray-TeV spectral evolution of the system as the pulsar passes through the Be star disk, and with the help of the received data to reconstruct the physical processes governing the system.
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