Chandra observations of the 2007 PSR B1259-63 periastron passage.

Physics

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Chandra Proposal Id #08400404

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 with 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 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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