Study of the Gamma-Ray Binary LS5039 with Suzaku

Details Study of the Gamma-Ray Binary LS5039 with Suzaku Study of the Gamma-Ray Binary LS5039 with Suzaku

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248..211t&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Astronomy and Astrophysics

Astronomy

Gamma-Ray Effects, Pulsars, Synchrotron Radiation, Binary Stars, Gamma-Ray, Pulsars, Synchrotron Radiation, Cataclysmic Binaries, Symbiotic Stars

Scientific paper

The Suzaku data of the galactic binary source LS 5039, which have continuous coverage of more than one orbital period, show strong modulation of the X-ray emission at the orbital period of this TeV gamma-ray emitting system. The X-ray radiation of LS 5039 is likely to be linked to very-high-energy electrons which are also responsible for the TeV gamma-ray emission.

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