Gamma-rays from the pulsar/Be star binary system PSR B1259-63/SS 2883

Details Gamma-rays from the pulsar/Be star binary system PSR B1259-63/SS 2883 Gamma-rays from the pulsar/Be star binary system PSR B1259-63/SS 2883

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..801..318s&link_type=abstract

ASTROPHYSICAL SOURCES OF HIGH ENERGY PARTICLES AND RADIATION. AIP Conference Proceedings, Volume 801, pp. 318-319 (2005).

Astronomy and Astrophysics

Astrophysics

1

Binary Stars, Pulsars, Variable Stars, Gamma-Ray Sources (Astronomical), Binary And Multiple Stars, Pulsars, Emission-Line Stars, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

The pulsar in PSR B1259-63/Be binary system injects relativistic e+/- pairs which lose energy on comptonization of thermal radiation from a massive companion and synchrotron process. These leptons produce γ-rays when propagating at the shock region formed in the interaction of the pulsar and stellar winds. We calculate the γ-ray light curve applying specific parameters of the binary system and structure of the stellar wind produced by the massive star.

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