- Conference date: 7–11 September 2009
- Location: Bologna (Italy)
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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