High Energy Emissions from the PSR1259-63/SS2883 Binary System

Details High Energy Emissions from the PSR1259-63/SS2883 Binary System High Energy Emissions from the PSR1259-63/SS2883 Binary System

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..745..353k&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astronomy

Pulsars, Binary And Multiple Stars, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

The PSR1259-63/SS2883 binary system consists of a Be star and a radio pulsar in a highly eccentric orbit. We discuss on very-high energy and high energy emissions from the particles accelerated in the Be star flows, due to the interactions of the relativistic pulsar wind and mass outflows of the star. The outflow parameters are constrained by the TeV observation results.

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